2,979 results on '"Zijlstra P"'
Search Results
152. Stellar Pulsation and the Production of Dust and Molecules in Galactic Carbon Stars
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Kraemer, Kathleen E., Sloan, G. C., Keller, Luke D., McDonald, Iain, Zijlstra, Albert A., and Groenewegen, Martin A. T.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
New infrared spectra of 33 Galactic carbon stars from FORCAST on SOFIA reveal strong connections between stellar pulsations and the dust and molecular chemistry in their circumstellar shells. A sharp boundary in overall dust content, which predominantly measures the amount of amorphous carbon, separates the semi-regular and Mira variables, with the semi-regulars showing little dust in their spectra and the Miras showing more. In semi-regulars, the contribution from SiC dust increases rapidly as the overall dust content grows, but in Miras, the SiC dust feature grows weaker as more dust is added. A similar dichotomy is found with the absorption band from CS at $\sim$7.3 $\mu$m, which is generally limited to semi-regular variables. Observationally, these differences make it straightforward to distinguish semi-regular and Mira variables spectroscopically without the need for long-term photometric observations or knowledge of their distances. The rapid onset of strong SiC emission in Galactic carbon stars in semi-regulars variables points to a different dust-condensation process before strong pulsations take over. The break in the production of amorphous carbon between semi-regulars and Miras seen in the Galactic sample is also evident in Magellanic carbon stars, linking strong pulsations in carbon stars to the strong mass-loss rates which will end their lives as stars across a wide range of metallicities., Comment: 22 pages, 13 figures, accepted by ApJ
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- 2019
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153. CO in the C1 globule of the Helix nebula with ALMA
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Andriantsaralaza, Miora, Zijlstra, Albert, and Avison, Adam
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
We present and analyse 12CO, 13CO and C18O(2-1) ALMA observations of the C1 globule inside the Helix nebula in order to determine its physical properties. Our findings confirm the molecular nature of the globule with a multi-peak structure. The 12CO line has a high optical depth of about 10. The derived 12C/13C ratio of 10 and 16O/18O ratio of 115 are not in agreement with the expected isotopic ratios of carbon-rich AGB stars. Assuming that the 12CO optical depth has been underestimated, we can find a consistent fit for an initial mass of 2 Msol. We obtain a molecular mass of 2x10-4 Msol for the C1 globule, which is much higher than its mass in the literature. Clumping could play a role in the high molecular mass of the knot. The origin of the tail is discussed. Our findings show that the most probable model appears to be shadowing. The kinematics and molecular morphology of the knot are not consistent with a wind-swept model and the photoevaporation model alone is not enough to explain the nature of the globule. We propose an integrated model where the effects of the photoevaporation, the stream and shadowing models are all considered in the tail shaping process., Comment: 17 pages, 12 figures, accepted for publication in MNRAS
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- 2019
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154. Circumstellar CO J = 3-2 detected around the evolving metal-poor ([Fe/H] ~ -1.15 dex) AGB star RU Vulpeculae
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McDonald, Iain, Uttenthaler, Stefan, Zijlstra, Albert A., Richards, Anita M. S., and Lagadec, Eric
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We report the first detection of CO J = 3-2 around a truly metal-poor evolved star. RU Vulpeculae is modelled to have Teff ~ 3620 K, L ~ 3128 +/- 516 L_Sun, log(g) = 0.0 ~ 0.2 dex and [Fe/H] = -1.3 to -1.0 dex, and is modelled to have recently undergone a thermal pulse. Its infrared flux has approximately doubled over 35 years. ALMA observations show the 3-2 line is narrow (half-width ~1.8-3.5 km/s). The 2-1 line is much weaker: it is not confidently detected. Spectral-energy-distribution fitting indicates very little circumstellar absorption, despite its substantial mid-infrared emission. A VISIR mid-infrared spectrum shows features typical of previously observed metal-poor stars, dominated by a substantial infrared excess but with weak silicate and (possibly) Al2O3 emission. A lack of resolved emission, combined with weak 2!1 emission, indicates the dense circumstellar material is truncated at large radii. We suggest that rapid dust condensation is occurring, but with an aspherical geometry (e.g., a disc or clumps) that does not obscure the star. We compare with T UMi, a similar star which is currently losing its dust., Comment: Accepted MNRAS, 16 pages, 7 figures
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- 2019
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155. Asymptotic Giant Branch Stars in the Nearby Dwarf Galaxy Leo P
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Goldman, Steven R., Boyer, Martha L., McQuinn, Kristen B., Sloan, Greg C., McDonald, Iain, van Loon, Jacco Th., Zijlstra, Albert A., Hirschauer, Alec S., Skillman, Evan D., and Srinivasan, Sundar
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
We have conducted a highly sensitive census of the evolved-star population in the metal-poor dwarf galaxy Leo P and detected four asymptotic giant branch (AGB) star candidates. Leo P is one of the best examples of a nearby analog of high-redshift galaxies because of its primitive metal content (2% of the solar value), proximity, and isolated nature, ensuring a less complicated history. Using medium-band optical photometry from the Hubble Space Telescope (HST), we have classified the AGB candidates by their chemical type. We have identified one oxygen-rich source which appears to be dusty in both the HST and Spitzer observations. Its brightness, however, suggests it may be a planetary nebula or post-AGB object. We have also identified three carbon-rich candidates, one of which may be dusty. Follow-up observations are needed to confirm the nature of these sources and to study the composition of any dust that they produce. If dust is confirmed, these stars would likely be among the most metal-poor examples of dust-producing stars known and will provide valuable insight into our understanding of dust formation at high redshift., Comment: Accepted for publication in ApJ
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- 2019
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156. SMART tracking: Simultaneous anatomical imaging and real-time passive device tracking for MR-guided interventions
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Zijlstra, Frank, Viergever, Max A., and Seevinck, Peter R.
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Physics - Medical Physics ,Computer Science - Computer Vision and Pattern Recognition - Abstract
Purpose: This study demonstrates a proof of concept of a method for simultaneous anatomical imaging and real-time (SMART) passive device tracking for MR-guided interventions. Methods: Phase Correlation template matching was combined with a fast undersampled radial multi-echo acquisition using the white marker phenomenon after the first echo. In this way, the first echo provides anatomical contrast, whereas the other echoes provide white marker contrast to allow accurate device localization using fast simulations and template matching. This approach was tested on tracking of five 0.5 mm steel markers in an agarose phantom and on insertion of an MRI-compatible 20 Gauge titanium needle in ex vivo porcine tissue. The locations of the steel markers were quantitatively compared to the marker locations as found on a CT scan of the same phantom. Results: The average pairwise error between the MRI and CT locations was 0.30 mm for tracking of stationary steel spheres and 0.29 mm during motion. Qualitative evaluation of the tracking of needle insertions showed that tracked positions were stable throughout needle insertion and retraction. Conclusions: The proposed SMART tracking method provided accurate passive tracking of devices at high framerates, inclusion of real-time anatomical scanning, and the capability of automatic slice positioning. Furthermore, the method does not require specialized hardware and could therefore be applied to track any rigid metal device that causes appreciable magnetic field distortions.
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- 2019
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157. The Nearby Evolved Stars Survey: I. JCMT/SCUBA-2 Sub-millimetre detection of the detached shell of U Antliae
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Dharmawardena, Thavisha E., Kemper, Francisca, Srinivasan, Sundar, Scicluna, Peter, Marshall, Jonathan P., Wouterloot, Jan G. A., Greaves, Jane, Goldman, Steven R., van Loon, Jacco Th., Matsuura, Mikako, McDonald, Iain, He, Jinhua, Zijlstra, Albert A., Toalá, Jesús A., Wallström, Sofia H. J., Kim, Hyosun, Trejo, Alfonso, Ventura, Paolo, Lagadec, Eric, Boyer, Martha L., Liu, Tie, Rau, Gioia, Izumiura, Hideyuki, Cami, Jan, Holland, Wayne, Jones, Olivia, and Shinnaga, Hiroko
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
We present the highest resolution single-dish submillimetre observations of the detached shell source U Antliae to date. The observations were obtained at $450~\micron$ and $850~\micron$ with SCUBA-2 instrument on the James Clerk Maxwell Telescope as part of the Nearby Evolved Stars Survey. The emission at $850~\micron$ peaks at $40\arcsec$ with hints of a second peak seen at $\sim 20\arcsec$. The emission can be traced out to a radius of $56\arcsec$ at a $3\sigma$ level. The outer peak observed at $850~\micron$ aligns well with the peak observed at Herschel/PACS wavelengths. With the help of spectral energy distribution fitting and radiative transfer calculations of multiple-shell models for the circumstellar envelope, we explore the various shell structures and the variation of grain sizes along the in the circumstellar envelope. We determine a total shell dust mass of $(2.0 \pm 0.3) \times 10^{-5}$ M$_{\odot}$ and established that the thermal pulse which gave rise to the detached shell occurred 3500 $\pm$ 500 years ago., Comment: Accepted for publication in MNRAS
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- 2019
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158. Three dimensional dust mapping of 12 supernovae remnants in the Galactic anticentre
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Yu, Bin, Chen, B. Q., Jiang, B. W., and Zijlstra, A.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Solar and Stellar Astrophysics - Abstract
We present three dimensional (3D) dust mapping of 12 supernova remnants (SNRs) in the Galactic anti-center (Galactic longitude $l$ between 150\degr\ and 210\degr) based on a recent 3D interstellar extinction map. The dust distribution of the regions which cover the full extents in the radio continuum for the individual SNRs are discussed. Four SNRs show significant spatial coincidences between molecular clouds (MCs) revealed from the 3D extinction mapping and the corresponding radio features. The results confirm the interactions between these SNRs and their surrounding MCs. Based on these correlations, we provide new distance estimates of the four SNRs, G189.1+3.0 (IC443, $d=1729^{+116}_{-94} \rm \,pc$), G190.9-2.2 ($d=1036^{+17}_{-81} \rm \,pc$), G205.5+0.5 ($d=941^{+96}_{-94}$ or $1257^{+92}_{-101} \rm \,pc$) and G213.0-0.6 ($d=1146^{+79}_{-80} \rm \,pc$). In addition, we find indirect evidences of potential interactions between SNRs and MCs for three other SNRs. New distance constraints are also given for these three SNRs., Comment: 14 pages, 13 figures, accepted for publication in MNRAS
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- 2019
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159. A high-mass Planetary Nebula in a Galactic Open Cluster
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Fragkou, Vasiliki, Parker, Quentin, Zijlstra, Albert, Crause, Lisa, and Barker, Helen
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
Planetary Nebulae are the ionised ejected envelopes surrounding the remnant cores of dying stars. Theory predicts that main-sequence stars with one to about eight times the mass of our sun may eventually form planetary nebulae. Until now no example has been confirmed at the higher mass range. Here we report that planetary nebula BMP J1613-5406 is associated with Galactic star cluster NGC 6067. Stars evolving off the main sequence of this cluster have a mass around five solar masses. Confidence in the planetary nebula-cluster association comes from their tightly consistent radial velocities in a sightline with a steep velocity-distance gradient, common distances, reddening and location of the planetary nebula within the cluster boundary. This is an unprecedented example of a planetary nebular whose progenitor star mass is getting close to the theoretical lower limit of core-collapse supernova formation. It provides evidence supporting theoretical predictions that 5+ solar mass stars can form planetary nebulae. Further study should provide fresh insights into stellar and Galactic chemical evolution., Comment: 22 pages, 4 figures, 3 tables. Nature Astronomy
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- 2019
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160. Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction
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Decin, L., Homan, W., Danilovich, T., de Koter, A., Engels, D., Waters, L. B. F. M., Muller, S., Gielen, C., García-Hernández, D. A., Stancliffe, R. J., Sande, M. Vande, Molenberghs, G., Kerschbaum, F., Zijlstra, A. A., and Mellah, I. El
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Astrophysics - Solar and Stellar Astrophysics - Abstract
In 1981, the idea of a superwind that ends the life of cool giant stars was proposed. Extreme OH/IR-stars develop superwinds with the highest mass-loss rates known so far, up to a few 10^(-4) Msun/yr, informing our understanding of the maximum mass-loss rate achieved during the Asymptotic Giant Branch (AGB) phase. A condundrum arises whereby the observationally determined duration of the superwind phase is too short for these stars to become white dwarfs. Here, we report on the detection of spiral structures around two cornerstone extreme OH/IR-stars, OH26.5+0.6 and OH30.1-0.7, identifying them as wide binary systems. Hydrodynamical simulations show that the companion's gravitational attraction creates an equatorial density enhancement mimicking a short extreme superwind phase, thereby solving the decades-old conundrum. This discovery restricts the maximum mass-loss rate of AGB stars around the single-scattering radiation-pressure limit of a few 10^(-5) Msun/yr. This brings about crucial implications for nucleosynthetic yields, planet survival, and the wind-driving mechanism., Comment: Publication date: 25 February 2019 at 16:00h GMT
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- 2019
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161. CT synthesis from MR images for orthopedic applications in the lower arm using a conditional generative adversarial network
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Zijlstra, Frank, Willemsen, Koen, Florkow, Mateusz C., Sakkers, Ralph J. B., Weinans, Harrie H., van der Wal, Bart C. H., van Stralen, Marijn, and Seevinck, Peter R.
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Computer Science - Computer Vision and Pattern Recognition ,Electrical Engineering and Systems Science - Image and Video Processing - Abstract
Purpose: To assess the feasibility of deep learning-based high resolution synthetic CT generation from MRI scans of the lower arm for orthopedic applications. Methods: A conditional Generative Adversarial Network was trained to synthesize CT images from multi-echo MR images. A training set of MRI and CT scans of 9 ex vivo lower arms was acquired and the CT images were registered to the MRI images. Three-fold cross-validation was applied to generate independent results for the entire dataset. The synthetic CT images were quantitatively evaluated with the mean absolute error metric, and Dice similarity and surface to surface distance on cortical bone segmentations. Results: The mean absolute error was 63.5 HU on the overall tissue volume and 144.2 HU on the cortical bone. The mean Dice similarity of the cortical bone segmentations was 0.86. The average surface to surface distance between bone on real and synthetic CT was 0.48 mm. Qualitatively, the synthetic CT images corresponded well with the real CT scans and partially maintained high resolution structures in the trabecular bone. The bone segmentations on synthetic CT images showed some false positives on tendons, but the general shape of the bone was accurately reconstructed. Conclusions: This study demonstrates that high quality synthetic CT can be generated from MRI scans of the lower arm. The good correspondence of the bone segmentations demonstrates that synthetic CT could be competitive with real CT in applications that depend on such segmentations, such as planning of orthopedic surgery and 3D printing., Comment: This work has been accepted at the SPIE Medical Imaging 2019, Image Processing conference, paper 10949-54
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- 2019
162. Circumstellar CO in metal-poor stellar winds: the highly irradiated globular cluster star 47 Tucanae V3
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McDonald, Iain, Boyer, Martha L., Groenewegen, Martin A. T., Lagadec, Eric, Richards, Anita M. S., Sloan, Gregory C., and Zijlstra, Albert A.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
We report the first detection of circumstellar CO in a globular cluster. Observations with ALMA have detected the CO J=3-2 and SiO v=1 J=8-7 transitions at 345 and 344 GHz, respectively, around V3 in 47 Tucanae (NGC 104; [Fe/H] = -0.72 dex), a star on the asymptotic giant branch. The CO line is detected at 7 sigma at a rest velocity v_LSR = -40.6 km/s and expansion velocity of 3.2 +/- ~0.4 km/s. The brighter, asymmetric SiO line may indicate a circumstellar maser. The stellar wind is slow compared to similar Galactic stars, but the dust opacity remains similar to Galactic comparisons. We suggest that the mass-loss rate is set by the levitation of material into the circumstellar environment by pulsations, but that the terminal wind-expansion velocity is determined by radiation pressure on the dust: a pulsation-enhanced dust-driven wind. We suggest the metal-poor nature of the star decreases the grain size, slowing the wind and increasing its density and opacity. Metallic alloys at high altitudes above the photosphere could also provide an opacity increase. The CO line is weaker than expected from Galactic AGB stars, but its strength confirms a model that includes CO dissociation by the strong interstellar radiation field present inside globular clusters., Comment: 5 pages, accepted MNRAS Letters
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- 2019
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163. The Central Star of Planetary Nebula PHR 1315-6555 and its host Galactic Open Cluster AL 1
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Fragkou, V., Parker, Q. A., Zijlstra, A. A., Shaw, R., and Lykou, F.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
PHR 1315-6555 is a rare case of a Galactic Planetary Nebula that is a proven member of the Open Cluster AL 1. This allows its distance to be defined with precision and thus the accurate measurement of its physical characteristics along with the parameters of its Central Star (CS). In this work we use HST to detect this unique CS and constrain the cluster's physical parameters. Our results suggest that the cluster rests at a distance of $\sim$12 kpc, is highly reddened, and has an age of around 0.66 Gyrs and a turn-off mass of $\sim$2.2 M$_\odot$. Our deep Colour Magnitude Diagram (CMD) suggests that the metallicity of the cluster is subsolar (Z=0.006). Our photometric measurements indicate that the PN's core is a faint blue star close to the nebular apparent centre, with an observed dereddened visual VEGA magnitude of 21.82 $\pm$ 0.60. A significant contribution from any possible binary companion is unlikely but possible. Our results show that the CS has an effective Zanstra temperature of around 113 kK and a mass of 0.58 M$_\odot$ providing a unique additional point to the fundamental White Dwarf Initial-to-Final-Mass Relation., Comment: accepted for publication in MNRAS
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- 2019
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164. Self-learning analytical interatomic potential describing laser-excited silicon
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Bauerhenne, Bernd, Lipp, Vladimir P., Zier, Tobias, Zijlstra, Eeuwe S., and Garcia, Martin E.
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Condensed Matter - Materials Science - Abstract
We develop an electronic-temperature dependent interatomic potential $\Phi (T_\text{e})$ for unexcited and laser-excited silicon. The potential is designed to reproduce ab initio molecular dynamics simulations by requiring force- and energy matching for each time step. $\Phi (T_\text{e})$ has a simple and flexible analytical form, can describe all relevant interactions and is applicable for any kind of boundary conditions (bulk, thin films, clusters). Its overall shape is automatically adjusted by a self-learning procedure, which finally finds the global minimum in the parameter space. We show that $\Phi (T_\text{e})$ can reproduce all thermal and nonthermal features provided by ab initio simulations. We apply the potential to simulate laser-excited Si nanoparticles and find critical damping of their breathing modes due to nonthermal melting.
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- 2018
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165. Characterizing the Bone Marrow Environment in Advanced-Stage Myelofibrosis during Ruxolitinib Treatment Using PET/CT and MRI: A Pilot Study
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Stefanie Slot, Cristina Lavini, Gerben J. C. Zwezerijnen, Bouke J. H. Boden, J. Tim Marcus, Marc C. Huisman, Maqsood Yaqub, Ellis Barbé, Mariëlle J. Wondergem, Josée M. Zijlstra, Sonja Zweegman, and Pieter G. Raijmakers
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myelofibrosis ,MRI ,PET/CT ,diagnostic accuracy ,ruxolitinib ,Computer applications to medicine. Medical informatics ,R858-859.7 - Abstract
Current diagnostic criteria for myelofibrosis are largely based on bone marrow (BM) biopsy results. However, these have several limitations, including sampling errors. Explorative studies have indicated that imaging might form an alternative for the evaluation of disease activity, but the heterogeneity in BM abnormalities complicates the choice for the optimal technique. In our prospective diagnostic pilot study, we aimed to visualize all BM abnormalities in myelofibrosis before and during ruxolitinib treatment using both PET/CT and MRI. A random sample of patients was scheduled for examinations at baseline and after 6 and 18 months of treatment, including clinical and laboratory examinations, BM biopsies, MRI (T1-weighted, Dixon, dynamic contrast-enhanced (DCE)) and PET/CT ([15O]water, [18F]NaF)). At baseline, all patients showed low BM fat content (indicated by T1-weighted MRI and Dixon), increased BM blood flow (as measured by [15O]water PET/CT), and increased osteoblastic activity (reflected by increased skeletal [18F]NaF uptake). One patient died after the baseline evaluation. In the others, BM fat content increased to various degrees during treatment. Normalization of BM blood flow (as reflected by [15O]water PET/CT and DCE-MRI) occurred in one patient, who also showed the fastest clinical response. Vertebral [18F]NaF uptake remained stable in all patients. In evaluable cases, histopathological parameters were not accurately reflected by imaging results. A case of sampling error was suspected. We conclude that imaging results can provide information on functional processes and disease distribution throughout the BM. Differences in early treatment responses were especially reflected by T1-weighted MRI. Limitations in the gold standard hampered the evaluation of diagnostic accuracy.
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- 2023
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166. Immune activation of vaginal human Langerhans cells increases susceptibility to HIV-1 infection
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Nienke H. van Teijlingen, Julia Eder, Ramin Sarrami-Forooshani, Esther M. Zijlstra-Willems, Jan-Paul W. R. Roovers, Elisabeth van Leeuwen, Carla M. S. Ribeiro, and Teunis B. H. Geijtenbeek
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Medicine ,Science - Abstract
Abstract Vaginal inflammation increases the risk for sexual HIV-1 transmission but underlying mechanisms remain unclear. In this study we assessed the impact of immune activation on HIV-1 susceptibility of primary human vaginal Langerhans cells (LCs). Vaginal LCs isolated from human vaginal tissue expressed a broad range of TLRs and became activated after exposure to both viral and bacterial TLR ligands. HIV-1 replication was restricted in immature vaginal LCs as only low levels of infection could be detected. Notably, activation of immature vaginal LCs by bacterial TLR ligands increased HIV-1 infection, whereas viral TLR ligands were unable to induce HIV-1 replication in vaginal LCs. Furthermore, mature vaginal LCs transmitted HIV-1 to CD4 T cells. This study emphasizes the role for vaginal LCs in protection against mucosal HIV-1 infection, which is abrogated upon activation. Moreover, our data suggest that bacterial STIs can increase the risk of HIV-1 acquisition in women.
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- 2023
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167. Evaluation of a novel technology-supported fall prevention intervention – study protocol of a multi-centre randomised controlled trial in older adults at increased risk of falls
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Tobias Morat, Melina Snyders, Philipp Kroeber, Alice De Luca, Valentina Squeri, Martin Hochheim, Philipp Ramm, Annika Breitkopf, Michael Hollmann, and Wiebren Zijlstra
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Fall prevention ,Technology-based ,Randomised controlled trial ,RCT ,Robot device ,Geriatrics ,RC952-954.6 - Abstract
Abstract Background Increasing number of falls and fall-related injuries in an aging society give rise to the need for effective fall prevention and rehabilitation strategies. Besides traditional exercise approaches, new technologies show promising options for fall prevention in older adults. As a new technology-based approach, the hunova robot can support fall prevention in older adults. The objective of this study is to implement and evaluate a novel technology-supported fall prevention intervention using the hunova robot compared to an inactive control group. The presented protocol aims at introducing a two-armed, multi-centre (four sites) randomised controlled trial, evaluating the effects of this new approach on the number of falls and number of fallers as primary outcomes. Methods The full clinical trial incorporates community-dwelling older adults at risk of falls with a minimum age of 65 years. Including a one-year follow-up measurement, all participants are tested four times. The training programme for the intervention group comprises 24-32 weeks in which training sessions are scheduled mostly twice a week; the first 24 training sessions use the hunova robot, these are followed by a home-based programme of 24 training sessions. Fall-related risk factors as secondary endpoints are measured using the hunova robot. For this purpose, the hunova robot measures the participants’ performance in several dimensions. The test outcomes are input for the calculation of an overall score which indicates the fall risk. The hunova-based measurements are accompanied by the timed-up-and-go test as a standard test within fall prevention studies. Discussion This study is expected to lead to new insights which may help establish a new approach to fall prevention training for older adults at risk of falls. First positive results on risk factors can be expected after the first 24 training sessions using the hunova robot. As primary outcomes, the number of falls and fallers within the study (including the one-year follow-up period) are the most relevant parameters that should be positively influenced by our new approach to fall prevention. After the study completion, approaches to examine the cost-effectiveness and develop an implementation plan are relevant aspects for further steps. Trial registration German Clinical Trial Register (DRKS), ID: DRKS00025897. Prospectively registered 16 August 2021, https://drks.de/search/de/trial/DRKS00025897 .
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- 2023
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168. Wound drainage after arthroplasty and prediction of acute prosthetic joint infection: prospective data from a multicentre cohort study using a telemonitoring app
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H. Scheper, R. Mahdad, B. Elzer, C. Löwik, W. Zijlstra, T. Gosens, J. C. T. van der Lugt, R. J. P. van der Wal, R. W. Poolman, M. P. Somford, P. C. Jutte, P. K. Bos, R. E. Zwaan, R. G. H. H. Nelissen, L. G. Visser, and M. G. J. de Boer
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Orthopedic surgery ,RD701-811 - Abstract
Background: Differentiation between uncomplicated and complicated postoperative wound drainage after arthroplasty is crucial to prevent unnecessary reoperation. Prospective data about the duration and amount of postoperative wound drainage in patients with and without prosthetic joint infection (PJI) are currently absent. Methods: A multicentre cohort study was conducted to assess the duration and amount of wound drainage in patients after arthroplasty. During 30 postoperative days after arthroplasty, patients recorded their wound status in a previously developed wound care app and graded the amount of wound drainage on a 5-point scale. Data about PJI in the follow-up period were extracted from the patient files. Results: Of the 1019 included patients, 16 patients (1.6 %) developed a PJI. Minor wound drainage decreased from the first to the fourth postoperative week from 50 % to 3 %. Both moderate to severe wound drainage in the third week and newly developed wound drainage in the second week after a week without drainage were strongly associated with PJI (odds ratio (OR) 103.23, 95 % confidence interval (CI) 26.08 to 408.57, OR 80.71, 95 % CI 9.12 to 714.52, respectively). The positive predictive value (PPV) for PJI was 83 % for moderate to heavy wound drainage in the third week. Conclusion: Moderate to heavy wound drainage and persistent wound drainage were strongly associated with PJI. The PPV of wound drainage for PJI was high for moderate to heavy drainage in the third week but was low for drainage in the first week. Therefore, additional parameters are needed to guide the decision to reoperate on patients for suspected acute PJI.
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- 2023
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169. Designing Computer-Based Tests: Design Guidelines from Multimedia Learning Studied with Eye Tracking
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Dirkx, K. J. H., Skuballa, I., Manastirean-Zijlstra, C. S., and Jarodzka, H.
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The use of computer-based tests (CBTs), for both formative and summative purposes, has greatly increased over the past years. One major advantage of CBTs is the easy integration of multimedia. It is unclear, though, how to design such CBT environments with multimedia. The purpose of the current study was to examine whether guidelines for designing multimedia "instruction" based on the Cognitive Load Theory (CLT) and Cognitive Theory of Multimedia Learning (CTML) will yield similar effects in CBT. In a within-subject design, thirty-three vocational students completed a computer-based arithmetic exam, in which half of the items were presented in an original design format, and the other half was redesigned based on the CTML principles for instructional design (i.e., adapted format). Results showed that applying CTML principles to a CBT decreased the difficulty of the test items, i.e., students scored significantly higher on the adapted test items. Moreover, eye-tracking data showed that the adapted items required less visual search and increased attention for the question and answer. Finally, cognitive load, measured as silent pauses during a secondary think-aloud task, decreased. Mean fixation duration (a different indicator of cognitive load), however, did not significantly differ between adapted and original items. These results indicate that applying multimedia principles to CBTs can be beneficial. It seems to prevent cognitive overload and helps students to focus on important parts of the test items (e.g., the question), leading to better test results.
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- 2021
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170. Comparing lesion and feature selections to predict progression in newly diagnosed DLBCL patients with FDG PET/CT radiomics features
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Eertink, Jakoba J., Zwezerijnen, Gerben J. C., Cysouw, Matthijs C. F., Wiegers, Sanne E., Pfaehler, Elisabeth A. G., Lugtenburg, Pieternella J., van der Holt, Bronno, Hoekstra, Otto S., de Vet, Henrica C. W., Zijlstra, Josée M., and Boellaard, Ronald
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- 2022
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171. Immediate versus staged revascularisation of non-culprit arteries in patients with acute coronary syndrome: a systematic review and meta-analysis
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Vriesendorp, P. A., Wilschut, J. M., Diletti, R., Daemen, J., Kardys, I., Zijlstra, F., Van Mieghem, N. M., Bennett, J., Esposito, G., Sabate, M., and den Dekker, W. K.
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- 2022
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172. Dragon 1 Protocol Manuscript: Training, Accreditation, Implementation and Safety Evaluation of Portal and Hepatic Vein Embolization (PVE/HVE) to Accelerate Future Liver Remnant (FLR) Hypertrophy
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Korenblik, R., Olij, B., Aldrighetti, L. A., Hilal, M. Abu, Ahle, M., Arslan, B., van Baardewijk, L. J., Baclija, I., Bent, C., Bertrand, C. L., Björnsson, B., de Boer, M. T., de Boer, S. W., Bokkers, R. P. H., Rinkes, I. H. M. Borel, Breitenstein, S., Bruijnen, R. C. G., Bruners, P., Büchler, M. W., Camacho, J. C., Cappelli, A., Carling, U., Chan, B. K. Y., Chang, D. H., choi, J., Font, J. Codina, Crawford, M., Croagh, D., Cugat, E., Davis, R., De Boo, D. W., De Cobelli, F., De Wispelaere, J. F., van Delden, O. M., Delle, M., Detry, O., Díaz-Nieto, R., Dili, A., Erdmann, J. I., Fisher, O., Fondevila, C., Fretland, Å., Borobia, F. Garcia, Gelabert, A., Gérard, L., Giuliante, F., Gobardhan, P. D., Gómez, F., Grünberger, T., Grünhagen, D. J., Guitart, J., Hagendoorn, J., Heil, J., Heise, D., Herrero, E., Hess, G. F., Hoffmann, M. H., Iezzi, R., Imani, F., Nguyen, J., Jovine, E., Kalff, J. C., Kazemier, G., Kingham, T. P., Kleeff, J., Kollmar, O., Leclercq, W. K. G., Ben, S. Lopez, Lucidi, V., MacDonald, A., Madoff, D. C., Manekeller, S., Martel, G., Mehrabi, A., Mehrzad, H., Meijerink, M. R., Menon, K., Metrakos, P., Meyer, C., Moelker, A., Modi, S., Montanari, N., Navines, J., Neumann, U. P., Peddu, P., Primrose, J. N., Qu, X., Raptis, D., Ratti, F., Ridouani, F., Rogan, C., Ronellenfitsch, U., Ryan, S., Sallemi, C., Moragues, J. Sampere, Sandström, P., Sarriá, L., Schnitzbauer, A., Serenari, M., Serrablo, A., Smits, M. L. J., Sparrelid, E., Spüntrup, E., Stavrou, G. A., Sutcliffe, R. P., Tancredi, I., Tasse, J. C., Udupa, V., Valenti, D., Fundora, Y., Vogl, T. J., Wang, X., White, S. A., Wohlgemuth, W. A., Yu, D., Zijlstra, I. A. J., Binkert, C. A., Bemelmans, M. H. A., van der Leij, C., Schadde, E., and van Dam, R. M.
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- 2022
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173. Do Professional Perspectives on Evidence-Based Smoking Cessation Methods Align? A Delphi Study among Researchers and Healthcare Professionals
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Zijlstra, Daniëlle N., Hoving, Ciska, Bolman, Catherine, Muris, Jean W. M., and De Vries, Hein
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The use of evidence-based smoking cessation interventions (SCIs) can significantly increase the number of successful smoking cessation attempts. To obtain an overview of the knowledge and viewpoints on the effectiveness and use of SCIs, a three-round online Delphi study was conducted among researchers and primary care professionals (PCPs). The four objectives of this study are to gain an overview of (i) the criteria important for recommending SCIs, (ii) the perceptions of both groups on the effectiveness of SCIs, (iii) the factors to consider when counseling different (high-risk) groups of smokers and (iv) the perceptions of both groups on the use of e-cigarettes as an SCI. We found a high level of agreement within groups on which smoker characteristics should be considered when recommending an SCI to smokers. We also found that PCPs display a lower degree of consensus on the effectiveness of SCIs. Both groups see a value in the use of special protocols for different (high-risk) groups of patients, but the two groups did not reach consensus on the use of e-cigarettes as a means to quit. Making an inventory of PCPs' needs regarding SCIs and their usage may provide insight into how to facilitate a better uptake in the primary care setting.
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- 2021
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174. External validation: a simulation study to compare cross-validation versus holdout or external testing to assess the performance of clinical prediction models using PET data from DLBCL patients
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Jakoba J. Eertink, Martijn W. Heymans, Gerben J. C. Zwezerijnen, Josée M. Zijlstra, Henrica C. W. de Vet, and Ronald Boellaard
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Internal validation ,External validation ,Model performance ,CV-AUC ,Medical physics. Medical radiology. Nuclear medicine ,R895-920 - Abstract
Abstract Aim Clinical prediction models need to be validated. In this study, we used simulation data to compare various internal and external validation approaches to validate models. Methods Data of 500 patients were simulated using distributions of metabolic tumor volume, standardized uptake value, the maximal distance between the largest lesion and another lesion, WHO performance status and age of 296 diffuse large B cell lymphoma patients. These data were used to predict progression after 2 years based on an existing logistic regression model. Using the simulated data, we applied cross-validation, bootstrapping and holdout (n = 100). We simulated new external datasets (n = 100, n = 200, n = 500) and simulated stage-specific external datasets (1), varied the cut-off for high-risk patients (2) and the false positive and false negative rates (3) and simulated a dataset with EARL2 characteristics (4). All internal and external simulations were repeated 100 times. Model performance was expressed as the cross-validated area under the curve (CV-AUC ± SD) and calibration slope. Results The cross-validation (0.71 ± 0.06) and holdout (0.70 ± 0.07) resulted in comparable model performances, but the model had a higher uncertainty using a holdout set. Bootstrapping resulted in a CV-AUC of 0.67 ± 0.02. The calibration slope was comparable for these internal validation approaches. Increasing the size of the test set resulted in more precise CV-AUC estimates and smaller SD for the calibration slope. For test datasets with different stages, the CV-AUC increased as Ann Arbor stages increased. As expected, changing the cut-off for high risk and false positive- and negative rates influenced the model performance, which is clearly shown by the low calibration slope. The EARL2 dataset resulted in similar model performance and precision, but calibration slope indicated overfitting. Conclusion In case of small datasets, it is not advisable to use a holdout or a very small external dataset with similar characteristics. A single small testing dataset suffers from a large uncertainty. Therefore, repeated CV using the full training dataset is preferred instead. Our simulations also demonstrated that it is important to consider the impact of differences in patient population between training and test data, which may ask for adjustment or stratification of relevant variables.
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- 2022
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175. The effect of the Progressive Goal Attainment Program on cognitions, perceptions, and work participation of workers with chronic health problems: study protocol for a randomized controlled trial
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Mariska de Wit, Hendrika P. Zijlstra, Carel T. J. Hulshof, Sylvia J. van der Burg-Vermeulen, and Angela G. E. M. de Boer
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Progressive Goal Attainment Program ,PGAP ,Intervention ,Work participation ,Workability ,Cognitions ,Medicine (General) ,R5-920 - Abstract
Abstract Background Cognitions and perceptions of workers with chronic health problems, such as catastrophizing thoughts and fear-avoidance beliefs, can negatively influence work participation. The Progressive Goal Attainment Program (PGAP) is an intervention developed in Canada with the aim of decreasing limiting cognitions and perceptions and increasing work participation. The objective of this protocol article is to describe the design of a randomized controlled superiority trial to study whether PGAP is effective in decreasing limiting cognitions and perceptions and increasing workability and work participation of workers with chronic health problems in the Netherlands. Methods This study is a randomized controlled superiority trial with two (parallel) groups, in which workers on sick leave are randomly assigned to an intervention group (PGAP intervention) or to a waiting-list control group (care as usual). The PGAP intervention consists of a maximum of 10 weekly individual sessions provided by a trained PGAP professional in which the worker learns about staying active, planning activities, and setting goals. Participants in this risk-targeted behavioral activation intervention also learn to be more aware of their cognitions and perceptions and learn about solution-focused problem-solving skills in challenging situations. The primary outcome is the degree of catastrophizing. Secondary outcomes are other personal cognitions and perceptions (e.g., expectations regarding return to work, self-efficacy), health symptoms (e.g., fatigue, depression), work participation (e.g., sick leave status, work hours), and other work-related outcomes (e.g., workability, quality of working life). Discussion Although PGAP shows positive effects in Canada, we do not know whether this intervention is effective in the Netherlands. This study is the first randomized controlled trial to test the effect of PGAP on limiting cognitions and perceptions and on work participation of workers with chronic health problems in the Netherlands. If PGAP is effective it could be implemented in the Netherlands in order to stimulate workability and work participation of workers. Trial registration The protocol of this study is registered in the Netherlands Trial Register (NL9832) in October 2021.
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- 2022
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176. How to persuade more primary care professionals to adopt a valued smoking cessation referral aid: a cross-sectional study of facilitators and barriers
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Daniëlle N Zijlstra, Catherine AW Bolman, Jean WM Muris, and Hein de Vries
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Smoking cessation ,Evidence-based interventions ,General practice ,Primary care ,Nurse practitioners ,Medicine (General) ,R5-920 - Abstract
Abstract Background To study the factors associated with the intention of primary care professionals (PCPs) to use or not use a referral aid (RA) for selecting an evidence-based smoking cessation intervention (EBSCI). Methods Participants (n = 85) were recruited from June to September 2020 to complete an online questionnaire based on the I-Change Model to assess the factors associated with the adoption of RA. The differences between PCPs with (n = 37) and without (n = 48) the intention to adopt in terms of demographics, motivational factors, and post-motivational factors were subsequently assessed. Correlation and logistic regression analyses were conducted to investigate the factors associated with the intention to adopt. Results Both groups indicated that they highly appreciated the RA. However, PCPs without the intention to adopt expressed a more negative attitude towards the RA, experienced less social support, showed low self-efficacy, and encountered barriers such as lack of time and skills. The factors most strongly associated with the intention to adopt were advantages, disadvantages, self-efficacy, less barriers, working in a solo practice and age. Conclusions The adoption of RA can be facilitated in two ways. The first one is by increasing the added value of the tool through a second round of co-creation focusing on the adoptability of the RA in practice. The second approach is by communicating the added value of referring to EBSCIS and thereby using the RA by implementing it in smoking cessation training for PCPs, which could also help to improve the attitude, social support, self-efficacy, and perceived skills in terms of RA usage among PCPs. Impact This study is the first work in the Netherlands to investigate the willingness of PCPs to actively refer patients to other EBSCIs in addition to providing face-to-face counseling themselves. Trial registration The study was registered at the Netherlands Trial Register (NL7020, https://www.trialregister.nl/trial/7020 ).
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- 2022
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177. R-CEOP as first-line treatment for anthracycline-ineligible patients with diffuse large B-cell lymphoma
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Diana Al-Sarayfi, Frederik O. Meeuwes, Müjde Durmaz, Djamila E. Issa, Rolf E. Brouwer, Aart Beeker, Anna van Rhenen, Pim G. N. J. Mutsaers, Lara H. Böhmer, Marjolein W. M. van der Poel, Liane te Boome, Tom van Meerten, Martine E. D. Chamuleau, Josée M. Zijlstra, Mirian Brink, and Marcel Nijland
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Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Published
- 2022
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178. Perception of prognosis and health-related quality of life in patients with advanced cancer: results of a multicentre observational study (eQuiPe)
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Zijlstra, Myrte, van Roij, J., Henselmans, I., van Laarhoven, H. W. M., Creemers, G. J., Vreugdenhil, G., Kuip, E. J. M., van de Poll-Franse, L. V., and Raijmakers, N. J. H.
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- 2023
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179. The hardgrounds of the Turonian–Coniacian carbonates of the Bagh Group of central India
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Ruidas, Dhiren Kumar and Zijlstra, J J P
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- 2023
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180. Het meten van angst om te vallen met de Falls Efficacy Scale-International (FES-I). Achtergrond en psychometrische kenmerken
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G. I. J. M. Kempen, G. A. R. Zijlstra, and J. C. M. van Haastregt
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angst ,vallen ,ouderen ,psychometrie ,FES-I ,Medicine - Abstract
Angst om te vallen komt frequent voor bij ouderen. In het verleden zijn hiervoor verschillende meetmethoden ontwikkeld. Een bekend en veelgebruikt is de Falls Efficacy Scale (FES). De FES blijkt echter (a) met name gericht te zijn op slechter functionerende ouderen en op activiteiten binnenshuis en minder geschikt te zijn voor ouderen uit de algemene populatie, (b) geen betrekking te hebben op sociale activiteiten die verband kunnen houden met valangst, en (c) te zijn ontwikkeld vanuit Amerikaans perspectief waardoor een eenduidige vertaling in verschillende Europese talen wordt bemoeilijkt. Binnen het Prevention of Falls Network Europe (ProFaNE) is de 16-item Falls Efficacy Scale-International (FES-I) ontwikkeld om tegemoet te komen aan deze bezwaren. In dit artikel wordt de Nederlandse versie van de FES-I gepresenteerd en wordt verslag gedaan van de psychometrische kwaliteiten van de FES-I in een Nederlandse steekproef van 213 ouderen van 70 jaar en ouder. De FES-I blijkt unidimensioneel en intern consistent te zijn; de test-hertest betrouwbaarheid is goed. De samenhang met leeftijd, geslacht, valincidenten en bezorgdheid om te vallen wordt zoals verwacht aangetroffen. Het discriminerend vermogen van de FES-I is vergelijkbaar met de oorspronkelijke FES. Geconcludeerd kan worden dat de FES-I een betrouwbaar en valide instrument is om angst om te vallen bij ouderen vast te stellen. Toekomstig onderzoek zal moeten uitwijzen of de FES-I ook gevoeliger is dan de FES voor het vaststellen van veranderingen in angst om te vallen.
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- 2023
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181. P619: TRACKING DISEASE PARAMETERS BY MRD, CT AND PET IN FIRST LINE CLL PATIENTS TREATED WITH FIXED DURATION IBRUTINIB-VENETOCLAX; INTERIM ANALYSIS OF THE FIRST 30 PATIENTS IN HOVON 158/NEXT STEP TRIAL.
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Sabina Kersting, Mark-David Levin, Julie Dubois, Yvette van Norden, Johan Dobber, Yvonne Jauw, Anne-Marie van der Kevie-Kersemaekers, Clemens Mellink, Caspar Da Cunha-Bang, Leonie Van Desr Burg, Doreen Te Raa, Fransien de Boer, Jolanda Droogendijk, Cecile Idink, Koen De Heer, Marten Nijziel, Lidwine Tick, Inge Ludwig, Mathijs Silbermann, Aart Beeker, Mar Bellido, Ludo Evers, Gerben Zwezerijnen, Josée Zijlstra, Marcel Kap, Carsten Niemann, and Arnon Kater
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Diseases of the blood and blood-forming organs ,RC633-647.5 - Published
- 2023
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182. P1139: COMPARISON OF 6XR-CHOP21 VERSUS 6XR-CHOP+2R FOR ADVANCED-STAGE DIFFUSE LARGE B-CELL LYMPHOMA: A PROPENSITY SCORE WEIGHTED POPULATION-BASED ANALYSIS
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Carolien Maas, David van Klaveren, Mujde Durmaz, Otto Visser, Djamila Issa, Eduardus F.M. Posthuma, Josée Zijlstra, Martine Chamuleau, Pieternella Lugtenburg, Marie José Kersten, and Avinash Dinmohamed
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Diseases of the blood and blood-forming organs ,RC633-647.5 - Published
- 2023
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183. P1159: INFERIOR OUTCOME OF FRAIL AND UNFIT PATIENTS WITH DIFFUSE LARGE B-CELL LYMPHOMA TREATED WITH ATTENUATED R-CHOP
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Diana Al-Sarayfi, Mirian Brink, Martine E. D. Chamuleau, Rolf Brouwer, Roos van Rijn, Djamila Issa, Wendy Deenik, Gerwin Huls, Rogier Mous, Joost S.P. Vermaat, Josee M. Zijlstra, Tom van Meerten, and Marcel Nijland
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Diseases of the blood and blood-forming organs ,RC633-647.5 - Published
- 2023
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184. P1246: CELL TYPE IDENTIFICATION USING MULTIPLEX IMMUNOFLUORESCENCE (MIF) GUIDED MACHINE LEARNING IN DLBCL
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Guillaume Chhor, Samuel Vilchez, Patrick Chang, Tatiana Novitskaya, Cyrus Hedvat, Limin Yu, Murray Resnick, Kai Franze, Brizelle Aguilar, Mariya Barch, Raj Jesudason, Ben Trotter, Jacqueline Brosnan-Cashman, Yi Liu, Ilan Wapinski, Jennifer Giltnane, Stephanie Hennek, Andries Zijlstra, and Lisa Mcginnis
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Diseases of the blood and blood-forming organs ,RC633-647.5 - Published
- 2023
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185. Toll-like receptor 4 and Syk kinase shape dendritic cell-induced immune activation to major house dust mite allergens
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Stefanie Busold, Jaap H. Akkerdaas, Esther M. Zijlstra-Willems, Kees van der Graaf, Sander W. Tas, Esther C. de Jong, Ronald van Ree, and Teunis B. H. Geijtenbeek
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house dust mite allergy ,Der p 1 ,Der p 2 ,TLR4 ,Syk ,dendritic cell activation ,Medicine (General) ,R5-920 - Abstract
BackgroundHouse dust mite (HDM) is a major cause of respiratory allergic diseases. Dendritic cells (DCs) play a central role in orchestrating adaptive allergic immune responses. However, it remains unclear how DCs become activated by HDM. Biochemical functions of the major HDM allergens Der p 1 (cysteine protease) and Der p 2 (MD2-mimick) have been implicated to contribute to DC activation.MethodsWe investigated the immune activating potential of HDM extract and its major allergens Der p 1 and Der p 2 using monocyte-derived DCs (moDCs). Maturation and activation markers were monitored by flow cytometry and cytokine production by ELISA. Allergen depletion and proteinase K digestion were used to investigate the involvement of proteins, and in particular of the major allergens. Inhibitors of spleen tyrosine kinase (Syk), Toll-like receptor 4 (TLR4) and of C-type lectin receptors (CLRs) were used to identify the involved receptors. The contribution of endotoxins in moDC activation was assessed by their removal from HDM extract.ResultsHDM extract induced DC maturation and cytokine responses in contrast to the natural purified major allergens Der p 1 and Der p 2. Proteinase K digestion and removal of Der p 1 or Der p 2 did not alter the immune stimulatory capacity of HDM extract. Antibodies against the CLRs Dectin-1, Dectin-2, and DC-SIGN did not affect cytokine responses. In contrast, Syk inhibition partially reduced IL-6, IL-12 and completely blocked IL-10. Blocking TLR4 signaling reduced the HDM-induced IL-10 and IL-12p70 induction, but not IL-6, while endotoxin removal potently abolished the induced cytokine response.ConclusionOur data strongly suggest that HDM-induced DC activation is neither dependent on Der p 1 nor Der p 2, but depend on Syk and TLR4 activation, which might suggest a crosstalk between Syk and TLR4 pathways. Our data highlight that endotoxins play a potent role in immune responses targeting HDM.
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- 2023
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186. Predictors of discordance between fractional flow reserve (FFR) and diastolic pressure ratio (dPR) in intermediate coronary lesions
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Alessandra Scoccia, Tara Neleman, Annemieke C. Ziedses des Plantes, Frederik T.W. Groenland, Jurgen M R Ligthart, Wijnand K. den Dekker, Roberto Diletti, Jeroen Wilschut, Rutger Jan Nuis, Felix Zijlstra, Eric Boersma, Nicolas M Van Mieghem, and Joost Daemen
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Coronary physiology ,diastolic Pressure ratio ,Fractional flow reserve ,Non-hyperemic pressure ratio ,Discordance in coronary physiology ,Diseases of the circulatory (Cardiovascular) system ,RC666-701 - Abstract
Background: Recently, non-hyperemic pressure ratios (NHPRs) have been validated as a reliable alternative to fractional flow reserve (FFR). However, a discordance between FFR and NHPRs is observed in 20–25% of cases. The aim of this study is to evaluate predictors of discordance between FFR and diastolic Pressure ratio (dPR). Methods: PREDICT is a retrospective, single center, investigator-initiated study including 813 patients (1092vessels) who underwent FFR assessment of intermediate coronary lesions (angiographic 30%-80% stenosis). dPR was calculated using individual pressure waveforms and dedicated software. Clinical, angiographic and hemodynamic variables were compared between patients with concordant and discordant FFR and dPR values. Results: Median age was 65 (IQR:59–73) years and 70% were male. Hemodynamically significant lesions, as defined by FFR ≤ 0.80, and dPR ≤ 0.89, were identified in 29.6% and 30.3% of cases, respectively. Overall, FFR and dPR values were discordant in 22.1% patients (17.4% of the vessels). Discordance was related to FFR+/dPR- and FFR-/dPR + in 11.8% and 10.3% of patients, respectively.In case of FFR-dPR discordance, a higher prevalence of left anterior descending arteries lesions was observed (70.5% vs. 53.1%, p
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- 2023
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187. Measuring citizenship competences: Assessment of measurement invariance
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Lianne Hoek, Bonne Zijlstra, Anke Munniksma, and Anne Bert Dijkstra
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measurement invariance ,measurement equivalence ,citizenship education ,social outcomes ,citizenship competences ,Special aspects of education ,LC8-6691 ,Social sciences (General) ,H1-99 - Abstract
Highlights: • Standardised questionnaires are used to measure the outcomes of citizenship education. • A prerequisite for cross-group comparisons based on these questionnaires is an assessment of measurement invariance. • This study used data from 6035 students from 87 Dutch primary schools to examine the measurement invariance of citizenship knowledge, attitude, and skill across sex, socioeconomic position and migration background. • The measurement invariance was sufficient in most cases. • Periodic assessment of measurement invariance in instruments measuring citizenship competences is important due to the dynamic nature of the construct. Purpose: Standardised questionnaires are used to measure the outcomes of citizenship education. These outcomes are often compared across groups to document different outcomes, for example, between boys and girls. A prerequisite for cross-group comparisons is an assessment of measurement invariance. Methodology: This study used data from 6035 students from 87 Dutch primary schools to examine the measurement invariance of the Citizenship Competences Questionnaire (Ten Dam et al., 2011). Dutch schools use this questionnaire to gain insight into students’ citizenship knowledge, attitudes, and skills. Measurement invariance was assessed across sex, socioeconomic position, and migration background. Findings: Measurement invariance was sufficient in most cases, allowing for cross-group comparisons of associations between latent constructs and their indicators, and in some cases, for cross-group comparisons of the latent means. We conclude by emphasising that periodic assessment of measurement invariance in instruments measuring citizenship competences is important due to the dynamic nature of the construct.
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- 2023
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188. ALMA Detection of Masers and Dasars in the Hydrogen Recombination Lines of the Planetary Nebula Mz3
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Zulema Abraham, Pedro P. B. Beaklini, Isabel Aleman, Raghvendra Sahai, Albert Zijlstra, Stavros Akras, Denise R. Gonçalves, and Toshiya Ueta
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Planetary nebulae ,Interstellar masers ,Astrophysical masers ,Astrophysics ,QB460-466 - Abstract
The hydrogen recombination lines H30 α , H40 α , H42 α , H50 β , and H57 γ and the underlying bremsstrahlung continuum emission were detected with ALMA in the bipolar nebula Mz3. The source was not spatially resolved, but the velocity profile of the H30 α line shows clear indication of maser amplification, confirming previous reports of laser amplification in the far-infrared H recombination lines observed with Herschel Space Observatory. Comparison between the flux densities of the H50 β , H40 α , and H42 α lines show overcooling, or darkness amplification by stimulated absorption (dasar effect) at the LSR velocity of about −25 km s ^−1 , which constrains the density of the absorbing region to about 10 ^3 cm ^−3 . The H30 α line, on the other hand, presents maser lines at LSR velocities of −69 and −98 km s ^−1 , which indicates ionized gas with densities close to 10 ^7 cm ^−3 . Although the source of emission was not resolved, it was possible to find the central position of the images for each velocity interval, which resulted in a well defined position–velocity distribution.
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- 2024
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189. FAST Detection of OH Emission in the Carbon-rich Planetary Nebula NGC 7027
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Xu-Jia Ouyang, Yong Zhang, Chuan-Peng Zhang, Peng Jiang, Jun-ichi Nakashima, Xi Chen, Hai-Hua Qiao, Xu-Ying Zhang, Hao-Min Sun, Xiao-Hu Li, and Albert Zijlstra
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Astrophysical masers ,Hydroxyl masers ,Planetary nebulae ,Circumstellar masers ,Astrophysics ,QB460-466 - Abstract
We present the first detection of the ground-state OH emission line at 1612 MHz toward the prototypical carbon-rich planetary nebula (PN) NGC 7027, utilizing the newly installed ultrawideband (UWB) receiver of the Five-hundred-meter Aperture Spherical radio Telescope (FAST). This emission is likely to originate from the interface of the neutral shell and the ionized region. The other three ground-state OH lines at 1665, 1667, and 1721 MHz are observed in absorption and have velocities well matched with that of HCO ^+ absorption. We infer that the OH absorption is from the outer shell of NGC 7027, although the possibility that they are associated with a foreground cloud cannot be completely ruled out. All the OH lines exhibit a single blueshifted component with respect to the central star. The formation of OH in carbon-rich environments might be via photodissociation-induced chemical processes. Our observations offer significant constraints for chemical simulations, and they underscore the potent capability of the UWB receiver of FAST to search for nascent PNe.
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- 2024
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190. SMC-Last Extracted Photometry
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T. A. Kuchar, G. C. Sloan, D. R. Mizuno, Kathleen E. Kraemer, M. L. Boyer, Martin A. T. Groenewegen, O. C. Jones, F. Kemper, Iain McDonald, Joana M. Oliveira, Marta Sewiło, Sundar Srinivasan, Jacco Th. van Loon, and Albert Zijlstra
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Small Magellanic Cloud ,Infrared photometry ,Celestial objects catalogs ,Astronomy ,QB1-991 - Abstract
We present point-source photometry from the Spitzer Space Telescope's final survey of the Small Magellanic Cloud (SMC). We mapped nearly 30 deg ^2 in two epochs in 2017, with the second extending to early 2018 at 3.6 and 4.5 μ m using the Infrared Array Camera. This survey duplicates the footprint from the SAGE-SMC program in 2008. Together, these surveys cover a nearly 10 yr temporal baseline in the SMC. We performed aperture photometry on the mosaicked maps produced from the new data. We did not use any prior catalogs as inputs for the extractor in order to be sensitive to any moving objects (e.g., foreground brown dwarfs) and other transient phenomena (e.g., cataclysmic variables or FU Ori–type eruptions). We produced a point-source catalog with high-confidence sources for each epoch as well as a combined-epoch catalog. For each epoch and the combined-epoch data, we also produced a more complete archive with lower-confidence sources. All of these data products will be made available to the community at the Infrared Science Archive.
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- 2024
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191. Prognostic value of post-percutaneous coronary intervention diastolic pressure ratio
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Masdjedi, K., van Zandvoort, L. J. C., Neleman, T., Kardys, I., Ligthart, J., Den Dekker, W. K., Diletti, R., Zijlstra, F., Van Mieghem, N. M., and Daemen, J.
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- 2022
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192. Impact of thrombus burden on long-term clinical outcomes in patients with either anterior or non-anterior ST-segment elevation myocardial infarction
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Scarparo, Paola, van Gameren, Menno, Wilschut, Jeroen, Daemen, Joost, Den Dekker, Wijnand K., Zijlstra, Felix, Van Mieghem, Nicolas M., and Diletti, Roberto
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- 2022
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193. An Imaging Spectroscopic Survey of the Planetary Nebula NGC 7009 with MUSE
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Walsh, J. R., Monreal-Ibero, A., Barlow, M. J., Ueta, T., Wesson, R., Zijlstra, A. A., Kimeswenger, S., Leal-Ferreira, M. L., and Otsuka, M.
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Astrophysics - Astrophysics of Galaxies - Abstract
The spatial structure of the emission lines and continuum over the 50 arcsecond extent of the nearby, O-rich, planetary nebula NGC 7009 (Saturn Nebula) have been observed with the MUSE integral field spectrograph on the ESO Very Large Telescope. Science Verification data, in <0.6 arcsecond seeing, have been reduced and analysed as images over the wavelength range 4750-9350A. Emission line maps over the bright shells are presented, from neutral to the highest ionization available (He II and [Mn V]). For collisionally excited lines (CELs), maps of electron temperature (T_e from [N II] and [S III]) and electron density (N_e from [S II] and [Cl III]) are available and for optical recombination lines (ORLs) temperature (from the Paschen jump and ratio of He I lines) and density (from high Paschen lines). These estimates are compared: for the first time, maps of the differences in CEL and ORL T_e's have been derived, and correspondingly a map of t^2 between a CEL and ORL temperature, showing considerable detail. Total abundances of He and O were formed, the latter using three ionization correction factors. However the map of He/H is not flat, departing by ~2% from a constant value, with remnants corresponding to ionization structures. Ionization correction factor methods are compared for O abundance, but none delivers a flat map. An integrated spectrum over an area of 2340 square arcseconds was also formed and compared to 1D photoionization models. The spatial variation of a range of nebular parameters illustrates the complexity of the ionized media in NGC 7009. These MUSE data are very rich with detections of many lines over areas of hundreds of square arcseconds and follow-on studies are indicated. (Abridged), Comment: Comments: 27 pages, 25 figures, 4 tables. Accepted for publication in A&A
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- 2018
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194. Pulsation-triggered dust production by asymptotic giant branch stars
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McDonald, Iain, de Beck, Elvire, Zijlstra, Albert A., and Lagadec, Eric
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Astrophysics - Solar and Stellar Astrophysics - Abstract
Eleven nearby (<300 pc), short-period (50-130 days) asymptotic giant branch (AGB) stars were observed in the CO J = (2-1) line. Detections were made towards objects that have evidence for dust production (Ks-[22] >~ 0.55 mag; AK Hya, V744 Cen, RU Crt, alpha Her). Stars below this limit were not detected (BQ Gem, eps Oct, NU Pav, II Hya, CL Hyi, ET Vir, SX Pav). Ks-[22] colour is found to trace mass-loss rate to well within an order of magnitude. This confirms existing results, indicating a factor of 100 increase in AGB-star mass-loss rates at a pulsation period of ~60 days, similar to the known "superwind" trigger at ~300 days. Between ~60 and ~300 days, an approximately constant mass-loss rate and wind velocity of ~3.7 x 10^-7 solar masses per year and ~8 km/s is found. While this has not been corrected for observational biases, this rapid increase in mass-loss rate suggests a need to recalibrate the treatment of AGB mass loss in stellar evolution models. The comparative lack of correlation between mass-loss rate and luminosity (for L <~ 6300 solar luminosities) suggests that the mass-loss rates of low-luminosity AGB-star winds are set predominantly by pulsations, not radiation pressure on dust, which sets only the outflow velocity. We predict that mass-loss rates from low-luminosity AGB stars, which exhibit optically thin winds, should be largely independent of metallicity, but may be strongly dependent on stellar mass., Comment: 18 pages, 7 figures, accepted for publication in MNRAS
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- 2018
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195. ALMA reveals the aftermath of a white dwarf--brown dwarf merger in CK Vulpeculae
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Eyres, Stewart, Evans, Aneurin, Zijlstra, Albert, Avison, Adam, Gehrz, Robert, Hajduk, Marcin, Starrfield, Sumner, Mohamed, Shazrene, Woodward, Charles, and Wagner, R. Mark
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We present Atacama Large Millimeter-Submillimeter Array (ALMA) observations of CK Vulpeculae which is identified with "Nova Vulpeculae 1670". They trace obscuring dust in the inner regions of the associated nebulosity. The dust forms two cocoons, each extending ~5 arcsec north and south of the presumed location of the central star. Brighter emission is in a more compact east-west structure (2 arcsec by 1 arcsec) where the cocoons intersect. We detect line emission in NH$_2$CHO, CN, four organic molecules and C$^{17}$O. CN lines trace bubbles within the dusty cocoons; CH$_3$OH a north-south S-shaped jet; and other molecules a central cloud with a structure aligned with the innermost dust structure. The major axis of the overall dust and gas bubble structure has a projected inclination of ~24 degrees with respect to a 71 arcsec extended "hourglass" nebulosity, previously seen in H alpha. Three cocoon limbs align with dark lanes in the inner regions of the same H alpha images. The central 2 arcsec by 1 arcsec dust is resolved into a structure consistent with a warped dusty disc. The velocity structure of the jets indicates an origin at the centre of this disc and precession with an unknown period. Deceleration regions at both the northern and southern tips of the jets are roughly coincident with additional diffuse dust emission over regions approximately 2 arcsec across. These structures are consistent with a bipolar outflow expanding into surrounding high density material. We suggest that a white dwarf and brown dwarf merged between 1670 and 1672, with the observed structures and extraordinary isotopic abundances generated as a result., Comment: 10 pages, 4 figures, accepted for publication in MNRAS 14th September 2018
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- 2018
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196. Central Stars of Planetary Nebulae in Galactic Open Clusters: Providing additional data for the White Dwarf Initial-to-Final-Mass Relation
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Fragkou, Vasiliki, Parker, Quentin A., Zijlstra, Albert, Shaw, Richard, and Lykou, Foteini
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Astrophysics - Solar and Stellar Astrophysics - Abstract
Accurate (<10%) distances of Galactic star clusters allow precise estimation of the physical parameters of any physically associated Planetary Nebula (PN) and also that of its central star (CSPN) and its progenitor. The progenitor's mass can be related to the PN's chemical characteristics and furthermore, provides additional data for the widely used white dwarf (WD) initial-to-final mass relation (IFMR) that is crucial for tracing the development of both carbon and nitrogen in entire galaxies. To date there is only one PN (PHR1315- 6555) confirmed to be physically associated with a Galactic open cluster (ESO 96 -SC04) that has a turn-off mass $\sim$2 M$_{\odot}$. Our deep HST photometry was used for the search of the CSPN of this currently unique PN. In this work, we present our results., Comment: 2 pages, 1 figure, IAU343 Synposium
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- 2018
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197. The curious case of II Lup: a complex morphology revealed with SAM/NACO and ALMA
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Lykou, Foteini, Zijlstra, Albert A., Kluska, Jacques, Lagadec, Eric, Tuthill, Peter G., Avison, Adam, Norris, Barnaby R. M., and Parker, Quentin A.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We present the first-ever images of the circumstellar environment of the carbon-rich AGB star II Lup in the infrared and sub-mm wavelengths, and the discovery of the envelope's non-spherical morphology with the use of high-angular resolution imaging techniques with the sparse aperture masking mode on NACO/VLT (that enables diffraction limited resolution from a single telescope) and with ALMA. We have successfully recovered images in $Ks$ (2.18$\mu$m), $L'$ (3.80$\mu$m) and $M'$ (4.78$\mu$m), that revealed the non-spherical morphology of the circumstellar envelope around II Lup. The stellar surface of the AGB star is unresolved (i.e. $\leq30$ mas in $Ks$) however the detected structure extends up to 110 mas from the star in all filters. Clumps have been found in the $Ks$ maps, while at lower emission levels a hook-like structure appears to extend counter-clockwise from the south. At larger spatial scales, the circumstellar envelope extends up to approximately 23 arcsec, while its shape suggests a spiral at four different molecules, namely CO, SiO, CS and HC$_3$N, with an average arm spacing of 1.7 arcsec which would imply an orbital period of 128 years for a distance of 590pc., Comment: 17 pages, 14 figures, accepted by MNRAS
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- 2018
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198. The Coordinated Radio and Infrared Survey for High-mass Star Formation. IV: A new radio selected sample of compact Galactic Planetary Nebulae
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Irabor, T., Hoare, M. G., Oudmaijer, R. D., Urquhart, J. S., Kurtz, S., Lumsden, S. L., Purcell, C. R., Zijlstra, A. A., and Umana, G.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
We present a new radio-selected sample of PNe from the CORNISH survey. This is a radio continuum survey of the inner Galactic plane covering Galactic longitude, $10^\circ
1000 K) and located closer than 7 kpc. Within this sample is a water-maser PN with a spectral index of $-0.55\pm 0.08$, which indicates non-thermal radio emission. Such a radio-selected sample, unaffected by extinction, will be particularly useful to compare with population synthesis models and should contribute to the understanding of the formation and evolution of PNe. - Published
- 2018
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199. Radio observations of planetary nebulae: no evidence for strong radial density gradients
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Hajduk, Marcin, van Hoof, Peter A. M., Śniadkowska, Karolina, Krankowski, Andrzej, Błaszkiewicz, Leszek, Dąbrowski, Bartosz, and Zijlstra, Albert A.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Radio continuum observations trace thermal emission of ionized plasma in planetary nebulae and bring useful information on nebular geometries. A model of homogeneous sphere or shell cannot fit the nebular spectra and brightness temperatures. Two alternative models have been proposed in the literature: the first one consists of two homogeneous components, while the other one is a model of a shell with a significant radial density gradient. On the other side, prolate ellipsoidal shell model can successfully fit the surface brightness distribution of selected objects. We verify the existing models using data collected in radio surveys covering wide range of frequencies. In about 50% cases, density gradient can be excluded, and none of the remaining objects could be confirmed. None of the observed planetary nebulae show the spectral index of 0.6 in the optically thick part of the spectrum, which is a value predicted for a shell containing strong radial density gradient. Radio spectra can be fitted with a model of prolate ellipsoidal shell, but also by a shell containing temperature variations in planetary nebulae. At least eight planetary nebulae show two component spectra, with one compact component showing much higher optical thickness than the other one. Unexpectedly, a group of planetary nebulae with lowest surface brightness show non-negligible optical thickness. Their emission comes from compact and dense structures, comprising only small part of total nebular mass., Comment: 22 pages, 20 figures
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- 2018
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200. Extended Dust Emission from Nearby Evolved Stars
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Dharmawardena, Thavisha E., Kemper, Francisca, Scicluna, Peter, Wouterloot, Jan G. A., Trejo, Alfonso, Srinivasan, Sundar, Cami, Jan, Zijlstra, Albert, and Marshall, Jonathan P.
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
We present JCMT SCUBA-2 $450\mu$m and $850\mu$m observations of 14 Asymptotic Giant Branch (AGB) stars (9 O--rich, 4 C-rich and 1 S--type) and one Red Supergiant (RSG) in the Solar Neighbourhood. We combine these observations with \emph{Herschel}/PACS observations at $70\mu$m and $160\mu$m and obtain azimuthally-averaged surface-brightness profiles and their PSF subtracted residuals. The extent of the SCUBA-2 850 $\mu$m emission ranges from 0.01 to 0.16 pc with an average of $\sim40\%$ of the total flux being emitted from the extended component. By fitting a modified black-body to the four-point SED at each point along the radial profile we derive the temperature ($T$), spectral index of dust emissivity ($\beta$) and dust column density ($\Sigma$) as a function of radius. For all the sources, the density profile deviates significantly from what is expected for a constant mass-loss rate, showing that all the sources have undergone variations in mass-loss during this evolutionary phase. In combination with results from CO line emission, we determined the dust-to-gas mass ratio for all the sources in our sample. We find that, when sources are grouped according to their chemistry, the resulting average dust-to-gas ratios are consistent with the respective canonical values. However we see a range of values with significant scatter which indicate the importance of including spatial information when deriving these numbers., Comment: 18 pages plus 13 pages of supplementary figures. Accepted for publication on MNRAS on 24/05/2018. Updated 05/07/2018: Fixed secondary axes (pc axes) on Radial Profiles in all figures
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- 2018
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