96 results on '"Benz, A. O."'
Search Results
2. STIX X-ray microflare observations during the Solar Orbiter commissioning phase
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Battaglia, Andrea Francesco, primary, Saqri, Jonas, additional, Massa, Paolo, additional, Perracchione, Emma, additional, Dickson, Ewan C. M., additional, Xiao, Hualin, additional, Veronig, Astrid M., additional, Warmuth, Alexander, additional, Battaglia, Marina, additional, Hurford, Gordon J., additional, Meuris, Aline, additional, Limousin, Olivier, additional, Etesi, László, additional, Maloney, Shane A., additional, Schwartz, Richard A., additional, Kuhar, Matej, additional, Schuller, Frederic, additional, Senthamizh Pavai, Valliappan, additional, Musset, Sophie, additional, Ryan, Daniel F., additional, Kleint, Lucia, additional, Piana, Michele, additional, Massone, Anna Maria, additional, Benvenuto, Federico, additional, Sylwester, Janusz, additional, Litwicka, Michalina, additional, Stȩślicki, Marek, additional, Mrozek, Tomasz, additional, Vilmer, Nicole, additional, Fárník, František, additional, Kašparová, Jana, additional, Mann, Gottfried, additional, Gallagher, Peter T., additional, Dennis, Brian R., additional, Csillaghy, André, additional, Benz, Arnold O., additional, and Krucker, Säm, additional
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- 2021
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3. ALMA small-scale features in the quiet Sun and active regions
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Brajsa, R., primary, Skokic, I., additional, Sudar, D., additional, Benz, A. O., additional, Krucker, S., additional, Ludwig, H.-G., additional, Saar, S. H., additional, and Selhorst, C. L., additional
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- 2021
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4. The Spectrometer/Telescope for Imaging X-rays (STIX)
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Krucker, Säm, primary, Hurford, G. J., additional, Grimm, O., additional, Kögl, S., additional, Gröbelbauer, H.-P, additional, Etesi, L., additional, Casadei, D., additional, Csillaghy, A., additional, Benz, A. O., additional, Arnold, N. G., additional, Molendini, F., additional, Orleanski, P., additional, Schori, D., additional, Xiao, H., additional, Kuhar, M., additional, Hochmuth, N., additional, Felix, S., additional, Schramka, F., additional, Marcin, S., additional, Kobler, S., additional, Iseli, L., additional, Dreier, M., additional, Wiehl, H. J., additional, Kleint, L., additional, Battaglia, M., additional, Lastufka, E., additional, Sathiapal, H., additional, Lapadula, K., additional, Bednarzik, M., additional, Birrer, G., additional, Stutz, St., additional, Wild, Ch., additional, Marone, F., additional, Skup, K. R., additional, Cichocki, A., additional, Ber, K., additional, Rutkowski, K., additional, Bujwan, W., additional, Juchnikowski, G., additional, Winkler, M., additional, Darmetko, M., additional, Michalska, M., additional, Seweryn, K., additional, Białek, A., additional, Osica, P., additional, Sylwester, J., additional, Kowalinski, M., additional, Ścisłowski, D., additional, Siarkowski, M., additional, Stęślicki, M., additional, Mrozek, T., additional, Podgórski, P., additional, Meuris, A., additional, Limousin, O., additional, Gevin, O., additional, Le Mer, I., additional, Brun, S., additional, Strugarek, A., additional, Vilmer, N., additional, Musset, S., additional, Maksimović, M., additional, Fárník, F., additional, Kozáček, Z., additional, Kašparová, J., additional, Mann, G., additional, Önel, H., additional, Warmuth, A., additional, Rendtel, J., additional, Anderson, J., additional, Bauer, S., additional, Dionies, F., additional, Paschke, J., additional, Plüschke, D., additional, Woche, M., additional, Schuller, F., additional, Veronig, A. M., additional, Dickson, E. C. M., additional, Gallagher, P. T., additional, Maloney, S. A., additional, Bloomfield, D. S., additional, Piana, M., additional, Massone, A. M., additional, Benvenuto, F., additional, Massa, P., additional, Schwartz, R. A., additional, Dennis, B. R., additional, van Beek, H. F., additional, Rodríguez-Pacheco, J., additional, and Lin, R. P., additional
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- 2020
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5. First analysis of solar structures in 1.21 mm full-disc ALMA image of the Sun
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Brajša, R., primary, Sudar, D., additional, Benz, A. O., additional, Skokić, I., additional, Bárta, M., additional, De Pontieu, B., additional, Kim, S., additional, Kobelski, A., additional, Kuhar, M., additional, Shimojo, M., additional, Wedemeyer, S., additional, White, S., additional, Yagoubov, P., additional, and Yan, Y., additional
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- 2018
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6. Water in star-forming regions with Herschel(WISH)
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Benz, A. O., Bruderer, S., van Dishoeck, E. F., Melchior, M., Wampfler, S. F., van der Tak, F., Goicoechea, J. R., Indriolo, N., Kristensen, L. E., Lis, D. C., Mottram, J. C., Bergin, E. A., Caselli, P., Herpin, F., Hogerheijde, M. R., Johnstone, D., Liseau, R., Nisini, B., Tafalla, M., Visser, R., and Wyrowski, F.
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ISM ultraviolet ,ISM molecules ,Massive stars ,Astrophysics::High Energy Astrophysical Phenomena ,Star formation ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Low-mass stars ,Astrophysics::Galaxy Astrophysics ,Astrochemistry - Abstract
CONTEXT: Hydrides are simple compounds containing one or a few hydrogen atoms bonded to a heavier atom. They are fundamental precursor molecules in cosmic chemistry and many hydride ions have become observable in high quality for the first time thanks to the Herschel Space Observatory. Ionized hydrides such as CH⁺ and OH⁺ (and also HCO⁺), which affect the chemistry of molecules such as water, provide complementary information on irradiation by far-UV (FUV) or X-rays and gas temperature. AIMS: We explore hydrides of the most abundant heavier elements in an observational survey covering young stellar objects (YSOs) with different mass and evolutionary state. The focus is on hydrides associated with the dense protostellar envelope and outflows, contrary to previous work that focused on hydrides in diffuse foreground clouds. METHODS: Twelve YSOs were observed with HIFI on Herschel in six spectral settings providing fully velocity-resolved line profiles as part of the Water in star-forming regions with Herschel (WISH) program. The YSOs include objects of low (Class 0 and I), intermediate, and high mass, with luminosities ranging from 4 L⊙ to 2 × 105 L⊙. RESULTS: The targeted lines of CH⁺, OH⁺, H₂O⁺+, C⁺, and CH are detected mostly in blue-shifted absorption. H₃O⁺ and SH⁺ are detected in emission and only toward some high-mass objects. The observed line parameters and correlations suggest two different origins related to gas entrained by the outflows and to the circumstellar envelope. The derived column densities correlate with bolometric luminosity and envelope mass for all molecules, best for CH, CH⁺, and HCO⁺. The column density ratios of CH⁺/OH⁺ are estimated from chemical slab models, assuming that the H₂ density is given by the specific density model of each object at the beam radius. For the low-mass YSOs the observed ratio can be reproduced for an FUV flux of 2–400 times the interstellar radiation field (ISRF) at the location of the molecules. In two high-mass objects, the UV flux is 20–200 times the ISRF derived from absorption lines, and 300–600 ISRF using emission lines. Upper limits for the X-ray luminosity can be derived from H₃O⁺ observations for some low-mass objects. CONCLUSIONS: If the FUV flux required for low-mass objects originates at the central protostar, a substantial FUV luminosity, up to 1.5 L⊙, is required. There is no molecular evidence for X-ray induced chemistry in the low-mass objects on the observed scales of a few 1000 AU. For high-mass regions, the FUV flux required to produce the observed molecular ratios is smaller than the unattenuated flux expected from the central object(s) at the Herschel beam radius. This is consistent with an FUV flux reduced by circumstellar extinction or by bloating of the protostar.
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- 2016
7. Water in star-forming regions with Herschel (WISH): VI. Constraints on UV and X-ray irradiation from a survey of hydrides in low- to high-mass young stellar objects
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Swiss National Science Foundation, Royal Netherlands Academy of Arts and Sciences, Netherlands Research School for Astronomy, National Aeronautics and Space Administration (US), European Research Council, Benz, A. O., Bruderer, S., Van Dishoeck, E. F., Melchior, M., Wampfler, S. F., Van Der Tak, F., Goicoechea, Javier R., Indriolo, N., Kristensen, L. E., Lis, D.C., Mottram, J.C., Bergin, E. A., Caselli, P., Herpin, F., Hogerheijde, M. R., Johnstone, D., Liseau, R., Nisini, B., Tafalla, M., Visser, R., Wyrowski, F., Swiss National Science Foundation, Royal Netherlands Academy of Arts and Sciences, Netherlands Research School for Astronomy, National Aeronautics and Space Administration (US), European Research Council, Benz, A. O., Bruderer, S., Van Dishoeck, E. F., Melchior, M., Wampfler, S. F., Van Der Tak, F., Goicoechea, Javier R., Indriolo, N., Kristensen, L. E., Lis, D.C., Mottram, J.C., Bergin, E. A., Caselli, P., Herpin, F., Hogerheijde, M. R., Johnstone, D., Liseau, R., Nisini, B., Tafalla, M., Visser, R., and Wyrowski, F.
- Abstract
[Context] Hydrides are simple compounds containing one or a few hydrogen atoms bonded to a heavier atom. They are fundamental precursor molecules in cosmic chemistry and many hydride ions have become observable in high quality for the first time thanks to the Herschel Space Observatory. Ionized hydrides such as CH+ and OH+ (and also HCO+), which affect the chemistry of molecules such as water, provide complementary information on irradiation by far-UV (FUV) or X-rays and gas temperature., [Aims] We explore hydrides of the most abundant heavier elements in an observational survey covering young stellar objects (YSOs) with different mass and evolutionary state. The focus is on hydrides associated with the dense protostellar envelope and outflows, contrary to previous work that focused on hydrides in diffuse foreground clouds., [Methods] Twelve YSOs were observed with HIFI on Herschel in six spectral settings providing fully velocity-resolved line profiles as part of the Water in star-forming regions with Herschel (WISH) program. The YSOs include objects of low (Class 0 and I), intermediate, and high mass, with luminosities ranging from 4 L⊙ to 2 × 105 L⊙., [Results] The targeted lines of CH+, OH+, H2O+, C+, and CH are detected mostly in blue-shifted absorption. H3O+ and SH+ are detected in emission and only toward some high-mass objects. The observed line parameters and correlations suggest two different origins related to gas entrained by the outflows and to the circumstellar envelope. The derived column densities correlate with bolometric luminosity and envelope mass for all molecules, best for CH, CH+, and HCO+. The column density ratios of CH+/OH+ are estimated from chemical slab models, assuming that the H2 density is given by the specific density model of each object at the beam radius. For the low-mass YSOs the observed ratio can be reproduced for an FUV flux of 2–400 times the interstellar radiation field (ISRF) at the location of the molecules. In two high-mass objects, the UV flux is 20–200 times the ISRF derived from absorption lines, and 300–600 ISRF using emission lines. Upper limits for the X-ray luminosity can be derived from H3O+ observations for some low-mass objects., [Conclusions] If the FUV flux required for low-mass objects originates at the central protostar, a substantial FUV luminosity, up to 1.5 L⊙, is required. There is no molecular evidence for X-ray induced chemistry in the low-mass objects on the observed scales of a few 1000 AU. For high-mass regions, the FUV flux required to produce the observed molecular ratios is smaller than the unattenuated flux expected from the central object(s) at the Herschel beam radius. This is consistent with an FUV flux reduced by circumstellar extinction or by bloating of the protostar.
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- 2016
8. Water in star-forming regions withHerschel(WISH)
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Benz, A. O., primary, Bruderer, S., additional, van Dishoeck, E. F., additional, Melchior, M., additional, Wampfler, S. F., additional, van der Tak, F., additional, Goicoechea, J. R., additional, Indriolo, N., additional, Kristensen, L. E., additional, Lis, D. C., additional, Mottram, J. C., additional, Bergin, E. A., additional, Caselli, P., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Johnstone, D., additional, Liseau, R., additional, Nisini, B., additional, Tafalla, M., additional, Visser, R., additional, and Wyrowski, F., additional
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- 2016
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9. First analysis of solar structures in 1.21mm full-disc ALMA image of the Sun.
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Brajša, R., Sudar, D., Benz, A. O., Skokić, I., Bárta, M., Pontieu, B. De, Kim, S., Kobelski, A., Kuhar, M., Shimojo, M., Wedemeyer, S., White, S., Yagoubov, P., and Yan, Y.
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SUN observations ,SUBMILLIMETER astronomy ,SOLAR atmosphere ,CORONAL holes - Abstract
Context. Various solar features can be seen in emission or absorption on maps of the Sun in the millimetre and submillimetre wavelength range. The recently installed Atacama Large Millimetre/submillimetre Array (ALMA) is capable of observing the Sun in that wavelength range with an unprecedented spatial, temporal and spectral resolution. To interpret solar observations with ALMA, the first important step is to compare solar ALMA maps with simultaneous images of the Sun recorded in other spectral ranges. Aims. The first aim of the present work is to identify different structures in the solar atmosphere seen in the optical, infrared, and EUV parts of the spectrum (quiet Sun, active regions, prominences on the disc, magnetic inversion lines, coronal holes and coronal bright points) in a full-disc solar ALMA image. The second aim is to measure the intensities (brightness temperatures) of those structures and to compare them with the corresponding quiet Sun level. Methods. A full-disc solar image at 1.21 mm obtained on December 18, 2015, during a CSV-EOC campaign with ALMA is calibrated and compared with full-disc solar images from the same day in Hα line, in He I 1083 nm line core, and with various SDO images (AIA at 170 nm, 30.4 nm, 21.1 nm, 19.3 nm, and 17.1 nm and HMI magnetogram). The brightness temperatures of various structures are determined by averaging over corresponding regions of interest in the calibrated ALMA image. Results. Positions of the quiet Sun, active regions, prominences on the disc, magnetic inversion lines, coronal holes and coronal bright points are identified in the ALMA image. At the wavelength of 1.21 mm, active regions appear as bright areas (but sunspots are dark), while prominences on the disc and coronal holes are not discernible from the quiet Sun background, despite having slightly less intensity than surrounding quiet Sun regions. Magnetic inversion lines appear as large, elongated dark structures and coronal bright points correspond to ALMA bright points. Conclusions. These observational results are in general agreement with sparse earlier measurements at similar wavelengths. The identification of coronal bright points represents the most important new result. By comparing ALMA and other maps, it was found that the ALMA image was oriented properly and that the procedure of overlaying the ALMA image with other images is accurate at the 5 arcsec level. The potential of ALMA for physics of the solar chromosphere is emphasised. [ABSTRACT FROM AUTHOR]
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- 2018
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10. Sensitive limits on the abundance of cold water vapor in the DM Tauri protoplanetary disk [Letter]
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Bergin, E. A., Hogerheijde, M. R., Brinch, C., Fogel, J., Yildiz, U. A., Kristensen, L. E., van Dishoeck, E. F., Bell, T. A., Blake, G. A., Cernicharo, J., Dominik, C., Lis, D., Melnick, G., Neufeld, D., Panic, O., Pearson, J. C., Bachiller, R., Baudry, A., Benedettini, M., Benz, A. O., Bjerkeli, P., Bontemps, S., Braine, J., Bruderer, S., Caselli, P., Codella, C., Daniel, F., di Giorgio, A. M., Doty, S. D., Encrenaz, P., Fich, M., Fuente, A., Giannini, T., Goicoechea, J. R., de Graauw, Th, Helmich, F., Herczeg, G. J., Herpin, F., Jacq, T., Johnstone, D., Jorgensen, J. K., Larsson, B., Liseau, R., Marseille, M., Mc Coey, C., Nisini, B., Olberg, M., Parise, Berengere, Plume, R., Risacher, C., Santiago-Garcia, J., Saraceno, P., Shipman, R., Tafalla, M., van Kempen, T. A., Visser, R., Wampfler, S. F., Wyrowski, F., van der Tak, F., Jellema, W., Tielens, A. G. G. M., Hartogh, P., Stuetzki, J., and Szczerba, R.
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QB - Abstract
We performed a sensitive search for the ground-state emission lines of ortho- and para-water vapor in the DM Tau protoplanetary disk using the Herschel/HIFI instrument. No strong lines are detected down to 3σ levels in 0.5 km s-1 channels of 4.2 mK for the 110–101 line and 12.6 mK for the 111–000 line. We report a very tentative detection, however, of the 110–101 line in the wide band spectrometer, with a strength of Tmb = 2.7 mK, a width of 5.6 km s-1 and an integrated intensity of 16.0 mK km s-1. The latter constitutes a 6σ detection. Regardless of the reality of this tentative detection, model calculations indicate that our sensitive limits on the line strengths preclude efficient desorption of water in the UV illuminated regions of the disk. We hypothesize that more than 95–99% of the water ice is locked up in coagulated grains that have settled to the midplane.
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- 2010
11. Water vapor toward starless cores: The Herschel view [Letter]
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Caselli, P., Keto, E., Pagani, L., Aikawa, Y., Yildiz, U. A., van der Tak, F. F. S., Tafalla, M., Bergin, E. A., Nisini, B., Codella, C., van Dishoeck, E. F., Bachiller, R., Baudry, A., Benedettini, M., Benz, A. O., Bjerkeli, P., Blake, G. A., Bontemps, S., Braine, J., Bruderer, S., Cernicharo, J., Daniel, F., di Giorgio, A. M., Dominik, C., Doty, S. D., Encrenaz, P., Fich, M., Fuente, A., Gaier, T., Giannini, T., Goicoechea, J. R., de Graauw, Th., Helmich, F., Herczeg, G. J., Herpin, F., Hogerheijde, M. R., Jackson, B., Jacq, T., Javadi, H., Johnstone, D., Jorgensen, J. K., Kester, D., Kristensen, L. E., Laauwen, W., Larsson, B., Lis, D., Liseau, R., Luinge, W., Marseille, M., McCoey, C., Megej, A., Melnick, G., Neufeld, D., Olberg, M., Parise, Berengere, Pearson, J. C., Plume, R., Risacher, C., Santiago-Garcia, J., Saraceno, P., Shipman, R., Siegel, P., van Kempen, T. A., Visser, R., Wampfler, S. F., and Wyrowski, F.
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QB - Abstract
Aims. Previous studies by the satellites SWAS and Odin provided stringent upper limits on the gas phase water abundance of dark clouds (x(H2O) < 7 × 10-9). We investigate the chemistry of water vapor in starless cores beyond the previous upper limits using the highly improved angular resolution and sensitivity of Herschel and measure the abundance of water vapor during evolutionary stages just preceding star formation.\ud Methods. High spectral resolution observations of the fundamental ortho water (o-H2O) transition (557 GHz) were carried out with the Heterodyne Instrument for the Far Infrared onboard Herschel toward two starless cores: Barnard 68 (hereafter B68), a Bok globule, and LDN 1544 (L1544), a prestellar core embedded in the Taurus molecular cloud complex. Detailed radiative transfer and chemical codes were used to analyze the data.\ud Results. The RMS in the brightness temperature measured for the B68 and L1544 spectra is 2.0 and 2.2 mK, respectively, in a velocity bin of 0.59 km s-1. The continuum level is 3.5 ± 0.2 mK in B68 and 11.4 ± 0.4 mK in L1544. No significant feature is detected in B68 and the 3σ upper limit is consistent with a column density of o-H2O N(o-H2O) < 2.5 × 1013 cm-2, or a fractional abundance x(o-H2O) < 1.3 × 10-9, more than an order of magnitude lower than the SWAS upper limit on this source. The L1544 spectrum shows an absorption feature at a 5σ level from which we obtain the first value of the o-H2O column density ever measured in dark clouds: N(o-H2O) = (8 ± 4) × 1012 cm-2. The corresponding fractional abundance is x(o-H2O) 5 × 10-9 at radii >7000 AU and 2 × 10-10 toward the center. The radiative transfer analysis shows that this is consistent with a x(o-H2O) profile peaking at 10-8, 0.1 pc away from the core center, where both freeze-out and photodissociation are negligible.\ud Conclusions. Herschel has provided the first measurement of water vapor in dark regions. Column densities of o-H2O are low, but prestellar cores such as L1544 (with their high central densities, strong continuum, and large envelopes) appear to be very promising tools to finally shed light on the solid/vapor balance of water in molecular clouds and oxygen chemistry in the earliest stages of star formation.
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- 2010
12. Water in star-forming regions withHerschel(WISH)(Corrigendum)
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Mottram, J. C., primary, Kristensen, L. E., additional, van Dishoeck, E. F., additional, Bruderer, S., additional, San José-García, I., additional, Karska, A., additional, Visser, R., additional, Santangelo, G., additional, Benz, A. O., additional, Bergin, E. A., additional, Caselli, P., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Johnstone, D., additional, van Kempen, T. A., additional, Liseau, R., additional, Nisini, B., additional, Tafalla, M., additional, van der Tak, F. F. S., additional, and Wyrowski, F., additional
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- 2015
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13. Water in star-forming regions withHerschel(WISH)
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Mottram, J. C., primary, Kristensen, L. E., additional, van Dishoeck, E. F., additional, Bruderer, S., additional, San José-García, I., additional, Karska, A., additional, Visser, R., additional, Santangelo, G., additional, Benz, A. O., additional, Bergin, E. A., additional, Caselli, P., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Johnstone, D., additional, van Kempen, T. A., additional, Liseau, R., additional, Nisini, B., additional, Tafalla, M., additional, van der Tak, F. F. S., additional, and Wyrowski, F., additional
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- 2014
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14. Dense molecular cocoons in the massive protocluster W3 IRS5: a test case for models of massive star formation
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Wang, K.-S., primary, Bourke, T. L., additional, Hogerheijde, M. R., additional, van der Tak, F. F. S., additional, Benz, A. O., additional, Megeath, S. T., additional, and Wilson, T. L., additional
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- 2013
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15. Observational evidence for dissociative shocks in the inner 100 AU of low-mass protostars usingHerschel-HIFI
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Kristensen, L. E., primary, van Dishoeck, E. F., additional, Benz, A. O., additional, Bruderer, S., additional, Visser, R., additional, and Wampfler, S. F., additional
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- 2013
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16. Water in star-forming regions withHerschel(WISH)
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van der Tak, F. F. S., primary, Chavarría, L., additional, Herpin, F., additional, Wyrowski, F., additional, Walmsley, C. M., additional, van Dishoeck, E. F., additional, Benz, A. O., additional, Bergin, E. A., additional, Caselli, P., additional, Hogerheijde, M. R., additional, Johnstone, D., additional, Kristensen, L. E., additional, Liseau, R., additional, Nisini, B., additional, and Tafalla, M., additional
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- 2013
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17. Water in star-forming regions withHerschel(WISH)
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Karska, A., primary, Herczeg, G. J., additional, van Dishoeck, E. F., additional, Wampfler, S. F., additional, Kristensen, L. E., additional, Goicoechea, J. R., additional, Visser, R., additional, Nisini, B., additional, San José-García, I., additional, Bruderer, S., additional, Śniady, P., additional, Doty, S., additional, Fedele, D., additional, Yıldız, U. A., additional, Benz, A. O., additional, Bergin, E., additional, Caselli, P., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Johnstone, D., additional, Jørgensen, J. K., additional, Liseau, R., additional, Tafalla, M., additional, van der Tak, F., additional, and Wyrowski, F., additional
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- 2013
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18. OH far-infrared emission from low- and intermediate-mass protostars surveyed withHerschel-PACS
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Wampfler, S. F., primary, Bruderer, S., additional, Karska, A., additional, Herczeg, G. J., additional, van Dishoeck, E. F., additional, Kristensen, L. E., additional, Goicoechea, J. R., additional, Benz, A. O., additional, Doty, S. D., additional, McCoey, C., additional, Baudry, A., additional, Giannini, T., additional, and Larsson, B., additional
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- 2013
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19. Water in star-forming regions withHerschel(WISH)
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Kristensen, L. E., primary, van Dishoeck, E. F., additional, Bergin, E. A., additional, Visser, R., additional, Yıldız, U. A., additional, San Jose-Garcia, I., additional, Jørgensen, J. K., additional, Herczeg, G. J., additional, Johnstone, D., additional, Wampfler, S. F., additional, Benz, A. O., additional, Bruderer, S., additional, Cabrit, S., additional, Caselli, P., additional, Doty, S. D., additional, Harsono, D., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Karska, A., additional, van Kempen, T. A., additional, Liseau, R., additional, Nisini, B., additional, Tafalla, M., additional, van der Tak, F., additional, and Wyrowski, F., additional
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- 2012
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20. Multi-line detection of O2towardρOphiuchi A
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Liseau, R., primary, Goldsmith, P. F., additional, Larsson, B., additional, Pagani, L., additional, Bergman, P., additional, Le Bourlot, J., additional, Bell, T. A., additional, Benz, A. O., additional, Bergin, E. A., additional, Bjerkeli, P., additional, Black, J. H., additional, Bruderer, S., additional, Caselli, P., additional, Caux, E., additional, Chen, J.-H., additional, de Luca, M., additional, Encrenaz, P., additional, Falgarone, E., additional, Gerin, M., additional, Goicoechea, J. R., additional, Hjalmarson, Å., additional, Hollenbach, D. J., additional, Justtanont, K., additional, Kaufman, M. J., additional, Le Petit, F., additional, Li, D., additional, Lis, D. C., additional, Melnick, G. J., additional, Nagy, Z., additional, Olofsson, A. O. H., additional, Olofsson, G., additional, Roueff, E., additional, Sandqvist, Aa., additional, Snell, R. L., additional, van der Tak, F. F. S., additional, van Dishoeck, E. F., additional, Vastel, C., additional, Viti, S., additional, and Yıldız, U. A., additional
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- 2012
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21. First hyperfine resolved far-infrared OH spectrum from a star-forming region
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Wampfler, S. F., primary, Bruderer, S., additional, Kristensen, L. E., additional, Chavarría, L., additional, Bergin, E. A., additional, Benz, A. O., additional, van Dishoeck, E. F., additional, Herczeg, G. J., additional, van der Tak, F. F. S., additional, Goicoechea, J. R., additional, Doty, S. D., additional, and Herpin, F., additional
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- 2011
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22. Herschel/HIFI spectroscopy of the intermediate mass protostar NGC 7129 FIRS 2
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Johnstone, D., primary, Fich, M., additional, McCoey, C., additional, van Kempen, T. A., additional, Fuente, A., additional, Kristensen, L. E., additional, Cernicharo, J., additional, Caselli, P., additional, Visser, R., additional, Plume, R., additional, Herczeg, G. J., additional, van Dishoeck, E. F., additional, Wampfler, S., additional, Bachiller, R., additional, Baudry, A., additional, Benedettini, M., additional, Bergin, E., additional, Benz, A. O., additional, Bjerkeli, P., additional, Blake, G., additional, Bontemps, S., additional, Braine, J., additional, Bruderer, S., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Doty, S. D., additional, Encrenaz, P., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Jacq, T., additional, Jørgensen, J. K., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Marseille, M., additional, Melnick, G., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Shipman, R., additional, Tafalla, M., additional, van der Tak, F., additional, Wyrowski, F., additional, Yıldız, U. A., additional, Caux, E., additional, Honingh, N., additional, Jellema, W., additional, Schieder, R., additional, Teyssier, D., additional, and Whyborn, N., additional
- Published
- 2010
- Full Text
- View/download PDF
23. Herschel/HIFI observations of high-JCO lines in the NGC 1333 low-mass star-forming region
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Yıldız, U. A., primary, van Dishoeck, E. F., additional, Kristensen, L. E., additional, Visser, R., additional, Jørgensen, J. K., additional, Herczeg, G. J., additional, van Kempen, T. A., additional, Hogerheijde, M. R., additional, Doty, S. D., additional, Benz, A. O., additional, Bruderer, S., additional, Wampfler, S. F., additional, Deul, E., additional, Bachiller, R., additional, Baudry, A., additional, Benedettini, M., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G. A., additional, Bontemps, S., additional, Braine, J., additional, Caselli, P., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herpin, F., additional, Jacq, T., additional, Johnstone, D., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Liu, F.-C., additional, Marseille, M., additional, McCoey, C., additional, Melnick, G., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Shipman, R., additional, Tafalla, M., additional, Tielens, A. G. G. M., additional, van der Tak, F., additional, Wyrowski, F., additional, Dieleman, P., additional, Jellema, W., additional, Ossenkopf, V., additional, Schieder, R., additional, and Stutzki, J., additional
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- 2010
- Full Text
- View/download PDF
24. Herschel/HIFI detections of hydrides towards AFGL 2591
- Author
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Bruderer, S., primary, Benz, A. O., additional, van Dishoeck, E. F., additional, Melchior, M., additional, Doty, S. D., additional, van der Tak, F., additional, Stäuber, P., additional, Wampfler, S. F., additional, Dedes, C., additional, Yıldız, U. A., additional, Pagani, L., additional, Giannini, T., additional, de Graauw, Th., additional, Whyborn, N., additional, Teyssier, D., additional, Jellema, W., additional, Shipman, R., additional, Schieder, R., additional, Honingh, N., additional, Caux, E., additional, Bächtold, W., additional, Csillaghy, A., additional, Monstein, C., additional, Bachiller, R., additional, Baudry, A., additional, Benedettini, M., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G. A., additional, Bontemps, S., additional, Braine, J., additional, Caselli, P., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Goicoechea, J. R., additional, Helmich, F., additional, Herczeg, G. J., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Jacq, T., additional, Johnstone, D., additional, Jørgensen, J. K., additional, Kristensen, L. E., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Marseille, M., additional, McCoey, C., additional, Melnick, G., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Tafalla, M., additional, van Kempen, T. A., additional, Visser, R., additional, and Wyrowski, F., additional
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- 2010
- Full Text
- View/download PDF
25. Variations in H2O+/H2O ratios toward massive star-forming regions
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Wyrowski, F., primary, van der Tak, F., additional, Herpin, F., additional, Baudry, A., additional, Bontemps, S., additional, Chavarria, L., additional, Frieswijk, W., additional, Jacq, T., additional, Marseille, M., additional, Shipman, R., additional, van Dishoeck, E. F, additional, Benz, A. O., additional, Caselli, P., additional, Hogerheijde, M. R., additional, Johnstone, D., additional, Liseau, R., additional, Bachiller, R., additional, Benedettini, M., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G., additional, Braine, J., additional, Bruderer, S., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Doty, S. D., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herczeg, G. J., additional, Jørgensen, J. K., additional, Kristensen, L. E., additional, Larsson, B., additional, Lis, D., additional, McCoey, C., additional, Melnick, G., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago, J., additional, Saraceno, P., additional, Tafalla, M., additional, van Kempen, T. A., additional, Visser, R., additional, Wampfler, S., additional, Yıldız, U. A., additional, Black, J. H., additional, Falgarone, E., additional, Gerin, M., additional, Roelfsema, P., additional, Dieleman, P., additional, Beintema, D., additional, De Jonge, A., additional, Whyborn, N., additional, Stutzki, J., additional, and Ossenkopf, V., additional
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- 2010
- Full Text
- View/download PDF
26. Herschelobservations of the hydroxyl radical (OH) in young stellar objects
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Wampfler, S. F., primary, Herczeg, G. J., additional, Bruderer, S., additional, Benz, A. O., additional, van Dishoeck, E. F., additional, Kristensen, L. E., additional, Visser, R., additional, Doty, S. D., additional, Melchior, M., additional, van Kempen, T. A., additional, Yıldız, U. A., additional, Dedes, C., additional, Goicoechea, J. R., additional, Baudry, A., additional, Melnick, G., additional, Bachiller, R., additional, Benedettini, M., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G. A., additional, Bontemps, S., additional, Braine, J., additional, Caselli, P., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, de Graauw, Th., additional, Helmich, F., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Jacq, T., additional, Johnstone, D., additional, Jørgensen, J. K., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Marseille, M., additional, Mc Coey, C., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Shipman, R., additional, Tafalla, M., additional, van der Tak, F. F. S., additional, Wyrowski, F., additional, Roelfsema, P., additional, Jellema, W., additional, Dieleman, P., additional, Caux, E., additional, and Stutzki, J., additional
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- 2010
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27. Gas morphology and energetics at the surface of PDRs: New insights withHerschelobservations of NGC 7023
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Joblin, C., primary, Pilleri, P., additional, Montillaud, J., additional, Fuente, A., additional, Gerin, M., additional, Berné, O., additional, Ossenkopf, V., additional, Le Bourlot, J., additional, Teyssier, D., additional, Goicoechea, J. R., additional, Le Petit, F., additional, Röllig, M., additional, Akyilmaz, M., additional, Benz, A. O., additional, Boulanger, F., additional, Bruderer, S., additional, Dedes, C., additional, France, K., additional, Güsten, R., additional, Harris, A., additional, Klein, T., additional, Kramer, C., additional, Lord, S. D., additional, Martin, P. G., additional, Martin-Pintado, J., additional, Mookerjea, B., additional, Okada, Y., additional, Phillips, T. G., additional, Rizzo, J. R., additional, Simon, R., additional, Stutzki, J., additional, van der Tak, F., additional, Yorke, H. W., additional, Steinmetz, E., additional, Jarchow, C., additional, Hartogh, P., additional, Honingh, C. E., additional, Siebertz, O., additional, Caux, E., additional, and Colin, B., additional
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- 2010
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- View/download PDF
28. Water abundances in high-mass protostellar envelopes:Herschelobservations with HIFI
- Author
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Marseille, M. G., primary, van der Tak, F. F. S., additional, Herpin, F., additional, Wyrowski, F., additional, Chavarría, L., additional, Pietropaoli, B., additional, Baudry, A., additional, Bontemps, S., additional, Cernicharo, J., additional, Jacq, T., additional, Frieswijk, W., additional, Shipman, R., additional, van Dishoeck, E. F., additional, Bachiller, R., additional, Benedettini, M., additional, Benz, A. O., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G. A., additional, Braine, J., additional, Bruderer, S., additional, Caselli, P., additional, Caux, E., additional, Codella, C., additional, Daniel, F., additional, Dieleman, P., additional, di Giorgio, A. M., additional, Dominik, C., additional, Doty, S. D., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Gaier, T., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herczeg, G. J., additional, Hogerheijde, M. R., additional, Jackson, B., additional, Javadi, H., additional, Jellema, W., additional, Johnstone, D., additional, Jørgensen, J. K., additional, Kester, D., additional, Kristensen, L. E., additional, Larsson, B., additional, Laauwen, W., additional, Lis, D., additional, Liseau, R., additional, Luinge, W., additional, McCoey, C., additional, Megej, A., additional, Melnick, G., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Roelfsema, P., additional, Santiago-García, J., additional, Saraceno, P., additional, Siegel, P., additional, Stutzki, J., additional, Tafalla, M., additional, van Kempen, T. A., additional, Visser, R., additional, Wampfler, S. F., additional, and Yıldız, U. A., additional
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- 2010
- Full Text
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29. Hydrides in young stellar objects: Radiation tracers in a protostar-disk-outflow system
- Author
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Benz, A. O., primary, Bruderer, S., additional, van Dishoeck, E. F., additional, Stäuber, P., additional, Wampfler, S. F., additional, Melchior, M., additional, Dedes, C., additional, Wyrowski, F., additional, Doty, S. D., additional, van der Tak, F., additional, Bächtold, W., additional, Csillaghy, A., additional, Megej, A., additional, Monstein, C., additional, Soldati, M., additional, Bachiller, R., additional, Baudry, A., additional, Benedettini, M., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G. A., additional, Bontemps, S., additional, Braine, J., additional, Caselli, P., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dieleman, P., additional, Dominik, C., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herczeg, G. J., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Jacq, T., additional, Jellema, W., additional, Johnstone, D., additional, Jørgensen, J. K., additional, Kristensen, L. E., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Marseille, M., additional, McCoey, C., additional, Melnick, G., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Ossenkopf, V., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Schieder, R., additional, Shipman, R., additional, Stutzki, J., additional, Tafalla, M., additional, Tielens, A. G. G. M., additional, van Kempen, T. A., additional, Visser, R., additional, and Yıldız, U. A., additional
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- 2010
- Full Text
- View/download PDF
30. Water in low-mass star-forming regions withHerschel
- Author
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Kristensen, L. E., primary, Visser, R., additional, van Dishoeck, E. F., additional, Yıldız, U. A., additional, Doty, S. D., additional, Herczeg, G. J., additional, Liu, F.-C., additional, Parise, B., additional, Jørgensen, J. K., additional, van Kempen, T. A., additional, Brinch, C., additional, Wampfler, S. F., additional, Bruderer, S., additional, Benz, A. O., additional, Hogerheijde, M. R., additional, Deul, E., additional, Bachiller, R., additional, Baudry, A., additional, Benedettini, M., additional, Bergin, E. A., additional, Bjerkeli, P., additional, Blake, G. A., additional, Bontemps, S., additional, Braine, J., additional, Caselli, P., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, de Graauw, Th., additional, di Giorgio, A. M., additional, Dominik, C., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, Goicoechea, J. R., additional, Helmich, F., additional, Herpin, F., additional, Jacq, T., additional, Johnstone, D., additional, Kaufman, M. J., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Marseille, M., additional, McCoey, C., additional, Melnick, G., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Shipman, R., additional, Tafalla, M., additional, Tielens, A. G. G. M., additional, van der Tak, F., additional, Wyrowski, F., additional, Beintema, D., additional, de Jonge, A., additional, Dieleman, P., additional, Ossenkopf, V., additional, Roelfsema, P., additional, Stutzki, J., additional, and Whyborn, N., additional
- Published
- 2010
- Full Text
- View/download PDF
31. Water in massive star-forming regions: HIFI observations of W3 IRS5
- Author
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Chavarría, L., primary, Herpin, F., additional, Jacq, T., additional, Braine, J., additional, Bontemps, S., additional, Baudry, A., additional, Marseille, M., additional, van der Tak, F., additional, Pietropaoli, B., additional, Wyrowski, F., additional, Shipman, R., additional, Frieswijk, W., additional, van Dishoeck, E. F., additional, Cernicharo, J., additional, Bachiller, R., additional, Benedettini, M., additional, Benz, A. O., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G. A., additional, Bruderer, S., additional, Caselli, P., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Doty, S. D., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Hartogh, P., additional, Helmich, F., additional, Herczeg, G. J., additional, Hogerheijde, M. R., additional, Johnstone, D., additional, Jørgensen, J. K., additional, Kristensen, L. E., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, McCoey, C., additional, Melnick, G., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Stutzki, J., additional, Szczerba, R., additional, Tafalla, M., additional, Tielens, A., additional, van Kempen, T. A., additional, Visser, R., additional, Wampfler, S. F., additional, Willem, J., additional, and Yıldız, U. A., additional
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- 2010
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- View/download PDF
32. Herschelspectral surveys of star-forming regions
- Author
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Ceccarelli, C., primary, Bacmann, A., additional, Boogert, A., additional, Caux, E., additional, Dominik, C., additional, Lefloch, B., additional, Lis, D., additional, Schilke, P., additional, van der Tak, F., additional, Caselli, P., additional, Cernicharo, J., additional, Codella, C., additional, Comito, C., additional, Fuente, A., additional, Baudry, A., additional, Bell, T., additional, Benedettini, M., additional, Bergin, E. A., additional, Blake, G. A., additional, Bottinelli, S., additional, Cabrit, S., additional, Castets, A., additional, Coutens, A., additional, Crimier, N., additional, Demyk, K., additional, Encrenaz, P., additional, Falgarone, E., additional, Gerin, M., additional, Goldsmith, P. F., additional, Helmich, F., additional, Hennebelle, P., additional, Henning, T., additional, Herbst, E., additional, Hily-Blant, P., additional, Jacq, T., additional, Kahane, C., additional, Kama, M., additional, Klotz, A., additional, Langer, W., additional, Lord, S., additional, Lorenzani, A., additional, Maret, S., additional, Melnick, G., additional, Neufeld, D., additional, Nisini, B., additional, Pacheco, S., additional, Pagani, L., additional, Parise, B., additional, Pearson, J., additional, Phillips, T., additional, Salez, M., additional, Saraceno, P., additional, Schuster, K., additional, Tielens, X., additional, van der Wiel, M. H. D., additional, Vastel, C., additional, Viti, S., additional, Wakelam, V., additional, Walters, A., additional, Wyrowski, F., additional, Yorke, H., additional, Liseau, R., additional, Olberg, M., additional, Szczerba, R., additional, Benz, A. O., additional, and Melchior, M., additional
- Published
- 2010
- Full Text
- View/download PDF
33. The origin of the [C II] emission in the S140 photon-dominated regions. New insights from HIFI
- Author
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Dedes, C., primary, Röllig, M., additional, Mookerjea, B., additional, Okada, Y., additional, Ossenkopf, V., additional, Bruderer, S., additional, Benz, A. O., additional, Melchior, M., additional, Kramer, C., additional, Gerin, M., additional, Güsten, R., additional, Akyilmaz, M., additional, Berne, O., additional, Boulanger, F., additional, De Lange, G., additional, Dubbeldam, L., additional, France, K., additional, Fuente, A., additional, Goicoechea, J. R., additional, Harris, A., additional, Huisman, R., additional, Jellema, W., additional, Joblin, C., additional, Klein, T., additional, Le Petit, F., additional, Lord, S., additional, Martin, P., additional, Martin-Pintado, J., additional, Neufeld, D. A., additional, Philipp, S., additional, Phillips, T., additional, Pilleri, P., additional, Rizzo, J. R., additional, Salez, M., additional, Schieder, R., additional, Simon, R., additional, Siebertz, O., additional, Stutzki, J., additional, van der Tak, F., additional, Teyssier, D., additional, and Yorke, H., additional
- Published
- 2010
- Full Text
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34. Herschelobservations in the ultracompact HII region Mon R2
- Author
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Fuente, A., primary, Berné, O., additional, Cernicharo, J., additional, Rizzo, J. R., additional, González-García, M., additional, Goicoechea, J. R., additional, Pilleri, P., additional, Ossenkopf, V., additional, Gerin, M., additional, Güsten, R., additional, Akyilmaz, M., additional, Benz, A. O., additional, Boulanger, F., additional, Bruderer, S., additional, Dedes, C., additional, France, K., additional, García-Burillo, S., additional, Harris, A., additional, Joblin, C., additional, Klein, T., additional, Kramer, C., additional, Le Petit, F., additional, Lord, S. D., additional, Martin, P. G., additional, Martín-Pintado, J., additional, Mookerjea, B., additional, Neufeld, D. A., additional, Okada, Y., additional, Pety, J., additional, Phillips, T. G., additional, Röllig, M., additional, Simon, R., additional, Stutzki, J., additional, van der Tak, F., additional, Teyssier, D., additional, Usero, A., additional, Yorke, H., additional, Schuster, K., additional, Melchior, M., additional, Lorenzani, A., additional, Szczerba, R., additional, Fich, M., additional, McCoey, C., additional, Pearson, J., additional, and Dieleman, P., additional
- Published
- 2010
- Full Text
- View/download PDF
35. HIFI observations of warm gas in DR21: Shock versus radiative heating
- Author
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Ossenkopf, V., primary, Röllig, M., additional, Simon, R., additional, Schneider, N., additional, Okada, Y., additional, Stutzki, J., additional, Gerin, M., additional, Akyilmaz, M., additional, Beintema, D., additional, Benz, A. O., additional, Berne, O., additional, Boulanger, F., additional, Bumble, B., additional, Coeur-Joly, O., additional, Dedes, C., additional, Diez-Gonzalez, M. C., additional, France, K., additional, Fuente, A., additional, Gallego, J. D., additional, Goicoechea, J. R., additional, Güsten, R., additional, Harris, A., additional, Higgins, R., additional, Jackson, B., additional, Jarchow, C., additional, Joblin, C., additional, Klein, T., additional, Kramer, C., additional, Lord, S., additional, Martin, P., additional, Martin-Pintado, J., additional, Mookerjea, B., additional, Neufeld, D. A., additional, Phillips, T., additional, Rizzo, J. R., additional, van der Tak, F. F. S., additional, Teyssier, D., additional, and Yorke, H., additional
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- 2010
- Full Text
- View/download PDF
36. Herschel-PACS spectroscopy of the intermediate mass protostar NGC 7129 FIRS 2
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Fich, M., primary, Johnstone, D., additional, van Kempen, T. A., additional, McCoey, C., additional, Fuente, A., additional, Caselli, P., additional, Kristensen, L. E., additional, Plume, R., additional, Cernicharo, J., additional, Herczeg, G. J., additional, van Dishoeck, E. F., additional, Wampfler, S., additional, Gaufre, P., additional, Gill, J. J., additional, Javadi, H., additional, Justen, M., additional, Laauwen, W., additional, Luinge, W., additional, Ossenkopf, V., additional, Pearson, J., additional, Bachiller, R., additional, Baudry, A., additional, Benedettini, M., additional, Bergin, E., additional, Benz, A. O., additional, Bjerkeli, P., additional, Blake, G., additional, Bontemps, S., additional, Braine, J., additional, Bruderer, S., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Doty, S. D., additional, Encrenaz, P., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herpin, F., additional, Hogerheijde, M. R., additional, Jacq, T., additional, Jørgensen, J. K., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Marseille, M., additional, Melnick, G., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Risacher, C., additional, Santiago, J., additional, Saraceno, P., additional, Shipman, R., additional, Tafalla, M., additional, van der Tak, F., additional, Visser, R., additional, Wyrowski, F., additional, and Yıldız, U. A., additional
- Published
- 2010
- Full Text
- View/download PDF
37. Water abundance variations around high-mass protostars: HIFI observations of the DR21 region
- Author
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van der Tak, F. F. S., primary, Marseille, M. G., additional, Herpin, F., additional, Wyrowski, F., additional, Baudry, A., additional, Bontemps, S., additional, Braine, J., additional, Doty, S., additional, Frieswijk, W., additional, Melnick, G., additional, Shipman, R., additional, van Dishoeck, E. F., additional, Benz, A. O., additional, Caselli, P., additional, Hogerheijde, M., additional, Johnstone, D., additional, Liseau, R., additional, Bachiller, R., additional, Benedettini, M., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G., additional, Bruderer, S., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, Goicoechea, J., additional, de Graauw, Th., additional, Helmich, F., additional, Herczeg, G., additional, Jørgensen, J., additional, Kristensen, L., additional, Larsson, B., additional, Lis, D., additional, McCoey, C., additional, Neufeld, D., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J., additional, Plume, R., additional, Risacher, C., additional, Santiago, J., additional, Saraceno, P., additional, Tafalla, M., additional, van Kempen, T., additional, Visser, R., additional, Wampfler, S., additional, Yıldız, U., additional, Ravera, L., additional, Roelfsema, P., additional, Siebertz, O., additional, and Teyssier, D., additional
- Published
- 2010
- Full Text
- View/download PDF
38. Strong CH+J= 1–0 emission and absorption in DR21
- Author
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Falgarone, E., primary, Ossenkopf, V., additional, Gerin, M., additional, Lesaffre, P., additional, Godard, B., additional, Pearson, J., additional, Cabrit, S., additional, Joblin, Ch., additional, Benz, A. O., additional, Boulanger, F., additional, Fuente, A., additional, Güsten, R., additional, Harris, A., additional, Klein, T., additional, Kramer, C., additional, Lord, S., additional, Martin, P., additional, Martin-Pintado, J., additional, Neufeld, D., additional, Phillips, T. G., additional, Röllig, M., additional, Simon, R., additional, Stutzki, J., additional, van der Tak, F., additional, Teyssier, D., additional, Yorke, H., additional, Erickson, N., additional, Fich, M., additional, Jellema, W., additional, Marston, A., additional, Risacher, C., additional, Salez, M., additional, and Schmülling, F., additional
- Published
- 2010
- Full Text
- View/download PDF
39. HIFI observations of water in the atmosphere of comet C/2008 Q3 (Garradd)
- Author
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Hartogh, P., primary, Crovisier, J., additional, de Val-Borro, M., additional, Bockelée-Morvan, D., additional, Biver, N., additional, Lis, D. C., additional, Moreno, R., additional, Jarchow, C., additional, Rengel, M., additional, Emprechtinger, M., additional, Szutowicz, S., additional, Banaszkiewicz, M., additional, Bensch, F., additional, Blecka, M. I., additional, Cavalié, T., additional, Encrenaz, T., additional, Jehin, E., additional, Küppers, M., additional, Lara, L.-M., additional, Lellouch, E., additional, Swinyard, B. M., additional, Vandenbussche, B., additional, Bergin, E. A., additional, Blake, G. A., additional, Blommaert, J. A. D. L., additional, Cernicharo, J., additional, Decin, L., additional, Encrenaz, P., additional, de Graauw, T., additional, Hutsemekers, D., additional, Kidger, M., additional, Manfroid, J., additional, Medvedev, A. S., additional, Naylor, D. A., additional, Schieder, R., additional, Thomas, N., additional, Waelkens, C., additional, Roelfsema, P. R., additional, Dieleman, P., additional, Güsten, R., additional, Klein, T., additional, Kasemann, C., additional, Caris, M., additional, Olberg, M., additional, and Benz, A. O., additional
- Published
- 2010
- Full Text
- View/download PDF
40. Water cooling of shocks in protostellar outflows
- Author
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Nisini, B., primary, Benedettini, M., additional, Codella, C., additional, Giannini, T., additional, Liseau, R., additional, Neufeld, D., additional, Tafalla, M., additional, van Dishoeck, E. F., additional, Bachiller, R., additional, Baudry, A., additional, Benz, A. O., additional, Bergin, E., additional, Bjerkeli, P., additional, Blake, G., additional, Bontemps, S., additional, Braine, J., additional, Bruderer, S., additional, Caselli, P., additional, Cernicharo, J., additional, Daniel, F., additional, Encrenaz, P., additional, di Giorgio, A. M., additional, Dominik, C., additional, Doty, S., additional, Fich, M., additional, Fuente, A., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herczeg, G., additional, Herpin, F., additional, Hogerheijde, M., additional, Jacq, T., additional, Johnstone, D., additional, Jørgensen, J., additional, Kaufman, M., additional, Kristensen, L., additional, Larsson, B., additional, Lis, D., additional, Marseille, M., additional, McCoey, C., additional, Melnick, G., additional, Olberg, M., additional, Parise, B., additional, Pearson, J., additional, Plume, R., additional, Risacher, C., additional, Santiago, J., additional, Saraceno, P., additional, Shipman, R., additional, van Kempen, T. A., additional, Visser, R., additional, Viti, S., additional, Wampfler, S., additional, Wyrowski, F., additional, van der Tak, F., additional, Yıldız, U. A., additional, Delforge, B., additional, Desbat, J., additional, Hatch, W. A., additional, Péron, I., additional, Schieder, R., additional, Stern, J. A., additional, Teyssier, D., additional, and Whyborn, N., additional
- Published
- 2010
- Full Text
- View/download PDF
41. TheHerschel-Heterodyne Instrument for the Far-Infrared (HIFI)
- Author
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de Graauw, Th., primary, Helmich, F. P., additional, Phillips, T. G., additional, Stutzki, J., additional, Caux, E., additional, Whyborn, N. D., additional, Dieleman, P., additional, Roelfsema, P. R., additional, Aarts, H., additional, Assendorp, R., additional, Bachiller, R., additional, Baechtold, W., additional, Barcia, A., additional, Beintema, D. A., additional, Belitsky, V., additional, Benz, A. O., additional, Bieber, R., additional, Boogert, A., additional, Borys, C., additional, Bumble, B., additional, Caïs, P., additional, Caris, M., additional, Cerulli-Irelli, P., additional, Chattopadhyay, G., additional, Cherednichenko, S., additional, Ciechanowicz, M., additional, Coeur-Joly, O., additional, Comito, C., additional, Cros, A., additional, de Jonge, A., additional, de Lange, G., additional, Delforges, B., additional, Delorme, Y., additional, den Boggende, T., additional, Desbat, J.-M., additional, Diez-González, C., additional, Di Giorgio, A. M., additional, Dubbeldam, L., additional, Edwards, K., additional, Eggens, M., additional, Erickson, N., additional, Evers, J., additional, Fich, M., additional, Finn, T., additional, Franke, B., additional, Gaier, T., additional, Gal, C., additional, Gao, J. R., additional, Gallego, J.-D., additional, Gauffre, S., additional, Gill, J. J., additional, Glenz, S., additional, Golstein, H., additional, Goulooze, H., additional, Gunsing, T., additional, Güsten, R., additional, Hartogh, P., additional, Hatch, W. A., additional, Higgins, R., additional, Honingh, E. C., additional, Huisman, R., additional, Jackson, B. D., additional, Jacobs, H., additional, Jacobs, K., additional, Jarchow, C., additional, Javadi, H., additional, Jellema, W., additional, Justen, M., additional, Karpov, A., additional, Kasemann, C., additional, Kawamura, J., additional, Keizer, G., additional, Kester, D., additional, Klapwijk, T. M., additional, Klein, Th., additional, Kollberg, E., additional, Kooi, J., additional, Kooiman, P.-P., additional, Kopf, B., additional, Krause, M., additional, Krieg, J.-M., additional, Kramer, C., additional, Kruizenga, B., additional, Kuhn, T., additional, Laauwen, W., additional, Lai, R., additional, Larsson, B., additional, Leduc, H. G., additional, Leinz, C., additional, Lin, R. H., additional, Liseau, R., additional, Liu, G. S., additional, Loose, A., additional, López-Fernandez, I., additional, Lord, S., additional, Luinge, W., additional, Marston, A., additional, Martín-Pintado, J., additional, Maestrini, A., additional, Maiwald, F. W., additional, McCoey, C., additional, Mehdi, I., additional, Megej, A., additional, Melchior, M., additional, Meinsma, L., additional, Merkel, H., additional, Michalska, M., additional, Monstein, C., additional, Moratschke, D., additional, Morris, P., additional, Muller, H., additional, Murphy, J. A., additional, Naber, A., additional, Natale, E., additional, Nowosielski, W., additional, Nuzzolo, F., additional, Olberg, M., additional, Olbrich, M., additional, Orfei, R., additional, Orleanski, P., additional, Ossenkopf, V., additional, Peacock, T., additional, Pearson, J. C., additional, Peron, I., additional, Phillip-May, S., additional, Piazzo, L., additional, Planesas, P., additional, Rataj, M., additional, Ravera, L., additional, Risacher, C., additional, Salez, M., additional, Samoska, L. A., additional, Saraceno, P., additional, Schieder, R., additional, Schlecht, E., additional, Schlöder, F., additional, Schmülling, F., additional, Schultz, M., additional, Schuster, K., additional, Siebertz, O., additional, Smit, H., additional, Szczerba, R., additional, Shipman, R., additional, Steinmetz, E., additional, Stern, J. A., additional, Stokroos, M., additional, Teipen, R., additional, Teyssier, D., additional, Tils, T., additional, Trappe, N., additional, van Baaren, C., additional, van Leeuwen, B.-J., additional, van de Stadt, H., additional, Visser, H., additional, Wildeman, K. J., additional, Wafelbakker, C. K., additional, Ward, J. S., additional, Wesselius, P., additional, Wild, W., additional, Wulff, S., additional, Wunsch, H.-J., additional, Tielens, X., additional, Zaal, P., additional, Zirath, H., additional, Zmuidzinas, J., additional, and Zwart, F., additional
- Published
- 2010
- Full Text
- View/download PDF
42. Detection of interstellar oxidaniumyl: Abundant H2O+towards the star-forming regions DR21, Sgr B2, and NGC6334
- Author
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Ossenkopf, V., primary, Müller, H. S. P., additional, Lis, D. C., additional, Schilke, P., additional, Bell, T. A., additional, Bruderer, S., additional, Bergin, E., additional, Ceccarelli, C., additional, Comito, C., additional, Stutzki, J., additional, Bacman, A., additional, Baudry, A., additional, Benz, A. O., additional, Benedettini, M., additional, Berne, O., additional, Blake, G., additional, Boogert, A., additional, Bottinelli, S., additional, Boulanger, F., additional, Cabrit, S., additional, Caselli, P., additional, Caux, E., additional, Cernicharo, J., additional, Codella, C., additional, Coutens, A., additional, Crimier, N., additional, Crockett, N. R., additional, Daniel, F., additional, Demyk, K., additional, Dieleman, P., additional, Dominik, C., additional, Dubernet, M. L., additional, Emprechtinger, M., additional, Encrenaz, P., additional, Falgarone, E., additional, France, K., additional, Fuente, A., additional, Gerin, M., additional, Giesen, T. F., additional, di Giorgio, A. M., additional, Goicoechea, J. R., additional, Goldsmith, P. F., additional, Güsten, R., additional, Harris, A., additional, Helmich, F., additional, Herbst, E., additional, Hily-Blant, P., additional, Jacobs, K., additional, Jacq, T., additional, Joblin, Ch., additional, Johnstone, D., additional, Kahane, C., additional, Kama, M., additional, Klein, T., additional, Klotz, A., additional, Kramer, C., additional, Langer, W., additional, Lefloch, B., additional, Leinz, C., additional, Lorenzani, A., additional, Lord, S. D., additional, Maret, S., additional, Martin, P. G., additional, Martin-Pintado, J., additional, McCoey, C., additional, Melchior, M., additional, Melnick, G. J., additional, Menten, K. M., additional, Mookerjea, B., additional, Morris, P., additional, Murphy, J. A., additional, Neufeld, D. A., additional, Nisini, B., additional, Pacheco, S., additional, Pagani, L., additional, Parise, B., additional, Pearson, J. C., additional, Pérault, M., additional, Phillips, T. G., additional, Plume, R., additional, Quin, S.-L., additional, Rizzo, R., additional, Röllig, M., additional, Salez, M., additional, Saraceno, P., additional, Schlemmer, S., additional, Simon, R., additional, Schuster, K., additional, van der Tak, F. F. S., additional, Tielens, A. G. G. M., additional, Teyssier, D., additional, Trappe, N., additional, Vastel, C., additional, Viti, S., additional, Wakelam, V., additional, Walters, A., additional, Wang, S., additional, Whyborn, N., additional, van der Wiel, M., additional, Yorke, H. W., additional, Yu, S., additional, and Zmuidzinas, J., additional
- Published
- 2010
- Full Text
- View/download PDF
43. Origin of the hot gas in low-mass protostars
- Author
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van Kempen, T. A., primary, Kristensen, L. E., additional, Herczeg, G. J., additional, Visser, R., additional, van Dishoeck, E. F., additional, Wampfler, S. F., additional, Bruderer, S., additional, Benz, A. O., additional, Doty, S. D., additional, Brinch, C., additional, Hogerheijde, M. R., additional, Jørgensen, J. K., additional, Tafalla, M., additional, Neufeld, D., additional, Bachiller, R., additional, Baudry, A., additional, Benedettini, M., additional, Bergin, E. A., additional, Bjerkeli, P., additional, Blake, G. A., additional, Bontemps, S., additional, Braine, J., additional, Caselli, P., additional, Cernicharo, J., additional, Codella, C., additional, Daniel, F., additional, di Giorgio, A. M., additional, Dominik, C., additional, Encrenaz, P., additional, Fich, M., additional, Fuente, A., additional, Giannini, T., additional, Goicoechea, J. R., additional, de Graauw, Th., additional, Helmich, F., additional, Herpin, F., additional, Jacq, T., additional, Johnstone, D., additional, Kaufman, M. J., additional, Larsson, B., additional, Lis, D., additional, Liseau, R., additional, Marseille, M., additional, McCoey, C., additional, Melnick, G., additional, Nisini, B., additional, Olberg, M., additional, Parise, B., additional, Pearson, J. C., additional, Plume, R., additional, Risacher, C., additional, Santiago-García, J., additional, Saraceno, P., additional, Shipman, R., additional, van der Tak, F., additional, Wyrowski, F., additional, Yıldız, U. A., additional, Ciechanowicz, M., additional, Dubbeldam, L., additional, Glenz, S., additional, Huisman, R., additional, Lin, R. H., additional, Morris, P., additional, Murphy, J. A., additional, and Trappe, N., additional
- Published
- 2010
- Full Text
- View/download PDF
44. Evidence of warm and dense material along the outflow of a high-mass YSO
- Author
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Bruderer, S., primary, Benz, A. O., additional, Bourke, T. L., additional, and Doty, S. D., additional
- Published
- 2009
- Full Text
- View/download PDF
45. Correlation between decimetric radio emission and hard X-rays in solar flares
- Author
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Dąbrowski, B. P., primary and Benz, A. O., additional
- Published
- 2009
- Full Text
- View/download PDF
46. Do solar decimetric spikes originate in coronal X-ray sources?
- Author
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Battaglia, M., primary and Benz, A. O., additional
- Published
- 2009
- Full Text
- View/download PDF
47. Observations of conduction driven evaporation in the early rise phase of solar flares
- Author
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Battaglia, M., primary, Fletcher, L., additional, and Benz, A. O., additional
- Published
- 2009
- Full Text
- View/download PDF
48. Heights of solar tracers observed at 8 mm and an interpretation of their radiation
- Author
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Brajša, R., primary, Romštajn, I., additional, Wöhl, H., additional, Benz, A. O., additional, Temmer, M., additional, and Roša, D., additional
- Published
- 2008
- Full Text
- View/download PDF
49. Observational evidence for return currents in solar flare loops
- Author
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Battaglia, M., primary and Benz, A. O., additional
- Published
- 2008
- Full Text
- View/download PDF
50. Energetic radiation and the sulfur chemistry of protostellar envelopes: submillimeter interferometry of AFGL 2591
- Author
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Benz, A. O., primary, Stäuber, P., additional, Bourke, T. L., additional, van der Tak, F. F. S., additional, van Dishoeck, E. F., additional, and Jørgensen, J. K., additional
- Published
- 2007
- Full Text
- View/download PDF
Catalog
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