21 results on '"Christina W. Li"'
Search Results
2. Controlled site coverage of strong metal–support interaction (SMSI) on Pd NP catalysts
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Christian J. Breckner, Kuixin Zhu, Mingrui Wang, Guanghui Zhang, Christina W. Li, and Jeffrey T. Miller
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Catalysis - Abstract
The coverage of Pd nanoparticles by SMSI oxides can be controlled with low loadings of TiO(2−x) and by controlling temperature in a reduction, oxidation, and re-reduction process.
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- 2023
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3. Haptophilicity and Substrate-Directed Reactivity in Diastereoselective Heterogeneous Hydrogenation
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Wei Hong, William A. Swann, Vamakshi Yadav, and Christina W. Li
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General Chemistry ,Catalysis - Published
- 2022
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4. Kinetic and Thermodynamic Factors Influencing Palladium Nanoparticle Redispersion into Mononuclear Pd(II) Cations in Zeolite Supports
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Trevor M. Lardinois, Keka Mandal, Vamakshi Yadav, Asanka Wijerathne, Brandon K. Bolton, Harrison Lippie, Christina W. Li, Christopher Paolucci, and Rajamani Gounder
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General Energy ,Physical and Theoretical Chemistry ,Surfaces, Coatings and Films ,Electronic, Optical and Magnetic Materials - Published
- 2022
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5. Heterogeneous Hydroxyl-Directed Hydrogenation: Control of Diastereoselectivity through Bimetallic Surface Composition
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Nicole J. Escorcia, Christina W. Li, William A. Swann, and Alexander J. Shumski
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inorganic chemicals ,010405 organic chemistry ,Chemistry ,Substrate (chemistry) ,General Chemistry ,010402 general chemistry ,01 natural sciences ,Combinatorial chemistry ,Catalysis ,0104 chemical sciences ,Bimetallic nanoparticle ,Homogeneous ,Composition (visual arts) ,Selectivity ,Bimetallic strip - Abstract
Directed hydrogenation, in which product selectivity is dictated by the binding of an ancillary directing group on the substrate to the catalyst, is typically catalyzed by homogeneous Rh and Ir com...
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- 2021
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6. Influence of the Defect Stability on n-Type Conductivity in Electron-Doped α- and β-Co(OH)2 Nanosheets
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Eve Y Martinez, Christina W. Li, and Kuixin Zhu
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010405 organic chemistry ,Brucite ,Chemistry ,Doping ,Oxide ,chemistry.chemical_element ,Crystal structure ,engineering.material ,010402 general chemistry ,01 natural sciences ,0104 chemical sciences ,Inorganic Chemistry ,Metal ,Crystallography ,chemistry.chemical_compound ,visual_art ,Vacancy defect ,engineering ,visual_art.visual_art_medium ,Physical and Theoretical Chemistry ,Cobalt ,Coordination geometry - Abstract
Electronic doping of transition-metal oxides (TMOs) is typically accomplished through the synthesis of nonstoichiometric oxide compositions and the subsequent ionization of intrinsic lattice defects. As a result, ambipolar doping of wide-band-gap TMOs is difficult to achieve because the formation energies and stabilities of vacancy and interstitial defects vary widely as a function of the oxide composition and crystal structure. The facile formation of lattice defects for one carrier type is frequently paired with the high-energy and unstable generation of defects required for the opposite carrier polarity. Previous work from our group showed that the brucite (β-phase) layered metal hydroxides of Co and Ni, intrinsically p-type materials in their anhydrous three-dimensional forms, could be n-doped using a strong chemical reductant. In this work, we extend the electron-doping study to the α polymorph of Co(OH)2 and elucidate the defects responsible for n-type doping in these two-dimensional materials. Through structural and electronic comparisons between the α, β, and rock-salt structures within the cobalt (hydr)oxide family of materials, we show that both layered structures exhibit facile formation of anion vacancies, the necessary defect for n-type doping, that are not accessible in the cubic CoO structure. However, the brucite polymorph is much more stable to reductive decomposition in the presence of doped electrons because of its tighter layer-to-layer stacking and octahedral coordination geometry, which results in a maximum conductivity of 10-4 S/cm, 2 orders of magnitude higher than the maximum value attainable on the α-Co(OH)2 structure.
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- 2021
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7. Superradiance and Exciton Delocalization in Perovskite Quantum Dot Superlattices
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Daria D. Blach, Victoria A. Lumsargis, Daniel E. Clark, Chern Chuang, Kang Wang, Letian Dou, Richard D. Schaller, Jianshu Cao, Christina W. Li, and Libai Huang
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Mechanical Engineering ,General Materials Science ,Bioengineering ,General Chemistry ,Condensed Matter Physics - Abstract
Achieving superradiance in solids is challenging due to fast dephasing processes from inherent disorder and thermal fluctuations. Perovskite quantum dots (QDs) are an exciting class of exciton emitters with large oscillator strength and high quantum efficiency, making them promising for solid-state superradiance. However, a thorough understanding of the competition between coherence and dephasing from phonon scattering and energetic disorder is currently unavailable. Here, we present an investigation of exciton coherence in perovskite QD solids using temperature-dependent photoluminescence line width and lifetime measurements. Our results demonstrate that excitons are coherently delocalized over 3 QDs at 11 K in superlattices leading to superradiant emission. Scattering from optical phonons leads to the loss of coherence and exciton localization to a single QD at temperatures above 100 K. At low temperatures, static disorder and defects limit exciton coherence. These results highlight the promise and challenge in achieving coherence in perovskite QD solids.
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- 2022
8. Controlling the Co–S coordination environment in Co-doped WS2 nanosheets for electrochemical oxygen reduction
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Wei Hong, Erika Meza, and Christina W. Li
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inorganic chemicals ,biology ,Renewable Energy, Sustainability and the Environment ,Chemistry ,Coordination number ,Active site ,chemistry.chemical_element ,02 engineering and technology ,General Chemistry ,Electrolyte ,Overpotential ,010402 general chemistry ,021001 nanoscience & nanotechnology ,Electrochemistry ,01 natural sciences ,Cobalt sulfide ,0104 chemical sciences ,Catalysis ,chemistry.chemical_compound ,Chemical engineering ,biology.protein ,General Materials Science ,0210 nano-technology ,Cobalt - Abstract
Cobalt sulfide nanomaterials are among the most active and stable catalysts for the electrocatalytic oxygen reduction reaction in pH 7 electrolyte. However, due to the complexity and dynamism of the catalytic surfaces in cobalt sulfide bulk materials, it is challenging to identify and tune the active site structure in order to achieve low overpotential oxygen reduction reactivity. In this work, we synthesize isolated Co sites supported on colloidal WS2 nanosheets and develop a synthetic strategy to rationally control the first-shell coordination environment surrounding the adsorbed Co active sites. By studying Co–WS2 materials with a range of Co–S coordination numbers, we are able to identify the optimal active site for pH 7 oxygen reduction catalysis, which comprises cobalt atoms bound to the WS2 support with a Co–S coordination number of 3–4. The optimized Co–WS2 material exhibits an oxygen reduction onset potential of 0.798 V vs. RHE, which is comparable to the most active bulk phases of cobalt sulfide in neutral electrolyte conditions.
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- 2021
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9. Modulating the Structure and Hydrogen Evolution Reactivity of Metal Chalcogenide Complexes through Ligand Exchange onto Colloidal Au Nanoparticles
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Jeffrey S. Lowe, Jeffrey Greeley, Eric Z. Liu, Alexander J. Shumski, Vamakshi Yadav, and Christina W. Li
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chemistry.chemical_compound ,chemistry ,Chemical engineering ,Ligand ,Chalcogenide ,Nanoparticle ,Reactivity (chemistry) ,General Chemistry ,Electrochemistry ,Molybdenum disulfide ,Catalysis ,Amorphous solid - Abstract
The interaction between catalyst and support is well known to influence the reactivity and stability of heterogeneous catalysts, and electrochemical hydrogen evolution catalysts based on amorphous ...
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- 2020
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10. Reversible Electron Doping of Layered Metal Hydroxide Nanoplates (M = Co, Ni) Using n-Butyllithium
- Author
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Christina W. Li, Eve Y Martinez, and Kuixin Zhu
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Materials science ,Metal hydroxide ,Mechanical Engineering ,Doping ,Inorganic chemistry ,Intercalation (chemistry) ,Oxide ,Bioengineering ,Electron donor ,02 engineering and technology ,General Chemistry ,021001 nanoscience & nanotechnology ,Condensed Matter Physics ,Metal ,chemistry.chemical_compound ,chemistry ,visual_art ,Vacancy defect ,visual_art.visual_art_medium ,Hydroxide ,General Materials Science ,0210 nano-technology - Abstract
Ambipolar doping of metal oxides is critical toward broadening the functionality of semiconducting oxides in electronic devices. Most metal oxides, however, show a strong preference for a single doping polarity due to the intrinsic stability of particular defects in an oxide lattice. In this work, we demonstrate that layered metal hydroxide nanomaterials of Co and Ni, which are intrinsically p-doped in their anhydrous rock salt form, can be n-doped using n-BuLi as a strong electron donor. A combination of X-ray characterization techniques reveal that hydroxide vacancy formation, Li+ adsorption, and varying degrees of electron delocalization are responsible for the stability of injected electrons. The doped electrons induce conductivity increases of 4-6 orders of magnitude relative to the undoped M(OH)2. We anticipate that chemical electron doping of layered metal hydroxides may be a general strategy to increase carrier concentration and stability for n-doping of intrinsically p-type metal oxides.
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- 2020
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11. Colloidal Synthesis of Well-Defined Bimetallic Nanoparticles for Nonoxidative Alkane Dehydrogenation
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Jeffrey T. Miller, Christina W. Li, Nicole J. Libretto, and Nicole J. Escorcia
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Alkane ,chemistry.chemical_classification ,010405 organic chemistry ,Chemistry ,Nanoparticle ,General Chemistry ,010402 general chemistry ,Heterogeneous catalysis ,01 natural sciences ,Combinatorial chemistry ,Catalysis ,0104 chemical sciences ,Dehydrogenation ,Well-defined ,Bimetallic strip ,Colloidal synthesis - Abstract
Precise synthesis and characterization of bimetallic nanoparticles are critical toward understanding structure–activity relationships in alkane dehydrogenation catalysis. Traditional synthetic meth...
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- 2020
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12. Solution-Phase Activation and Functionalization of Colloidal WS2 Nanosheets with Ni Single Atoms
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Erika Meza, Christina W. Li, and Rosa E. Diaz
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Materials science ,Tungsten disulfide ,General Engineering ,Oxygen evolution ,General Physics and Astronomy ,02 engineering and technology ,010402 general chemistry ,021001 nanoscience & nanotechnology ,01 natural sciences ,Solution phase ,0104 chemical sciences ,Catalysis ,Colloid ,chemistry.chemical_compound ,Chemical engineering ,chemistry ,Surface modification ,General Materials Science ,0210 nano-technology ,Colloidal synthesis - Abstract
Single-atom functionalization of transition-metal dichalcogenide (TMD) nanosheets is a powerful strategy to tune the optical, magnetic, and catalytic properties of two-dimensional materials. In thi...
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- 2020
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13. Surface functionalization of Pt nanoparticles with metal chlorides for bifunctional CO oxidation
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Christina W. Li and Eve Y Martinez
- Subjects
010405 organic chemistry ,Oxide ,Nanoparticle ,Overpotential ,010402 general chemistry ,01 natural sciences ,Catalyst poisoning ,0104 chemical sciences ,Catalysis ,Inorganic Chemistry ,chemistry.chemical_compound ,Adsorption ,Transition metal ,chemistry ,Chemical engineering ,Materials Chemistry ,Physical and Theoretical Chemistry ,Bifunctional - Abstract
Incorporation of a metal oxide or hydroxide species into Pt-based electrocatalysts has been shown to lower the overpotential required to oxidatively remove carbon monoxide from the catalyst surface, a reaction that is critical to preventing catalyst poisoning and deactivation in fuel cell devices. In this work, we report a general synthetic method toward Pt-metal oxide composite nanoparticles via the adsorption of metal halide ligands onto 1–2 nm colloidal Pt nanoparticles. Pt-metal oxide composite nanoparticles spanning across the first-row transition metals and post-transition metals are synthesized and characterized with transmission electron microscopy and energy dispersive X-ray scattering. CO stripping and steady-state CO oxidation experiments reveal that Mn, Fe, Co, Ni, and In oxides are capable of participating in the catalysis as a bifunctional partner and reduce the overpotential required for CO electrooxidation by ∼200 mV relative to pure Pt.
- Published
- 2019
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14. Microstructural Evolution of Au@Pt Core–Shell Nanoparticles under Electrochemical Polarization
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Wei Hong and Christina W. Li
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Materials science ,Nanoparticle ,02 engineering and technology ,010402 general chemistry ,021001 nanoscience & nanotechnology ,Microstructure ,Electrochemistry ,Electrocatalyst ,01 natural sciences ,0104 chemical sciences ,Catalysis ,Metal ,Chemical engineering ,visual_art ,visual_art.visual_art_medium ,General Materials Science ,0210 nano-technology ,Polarization (electrochemistry) ,Bimetallic strip - Abstract
Understanding the microstructural evolution of bimetallic Pt nanoparticles under electrochemical polarization is critical to developing durable fuel cell catalysts. In this work, we develop a colloidal synthetic method to generate core-shell Au@Pt nanoparticles of varying surface Pt coverages to understand how as-synthesized bimetallic microstructure influences nanoparticle structural evolution during formic acid oxidation. By comparing the electrochemical and structural properties of our Au@Pt core-shells with bimetallic AuPt alloys at various stages in catalytic cycling, we determine that these two structures evolve in divergent ways. In core-shell nanoparticles, Au atoms from the core migrate outward onto the surface, generating transient "single-atom" Pt active sites with high formic acid oxidation activity. Metal migration continues until Pt is completely encapsulated by Au, and catalytic reactivity ceases. In contrast, AuPt alloys undergo surface dealloying and significant leaching of Pt out of the nanoparticle. Elucidating the dynamic restructuring processes responsible for high electrocatalytic reactivity in Pt bimetallic structures will enable better design and predictive synthesis of nanoparticle catalysts that are both active and stable.
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- 2019
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15. Reversible Electron Doping of Layered Metal Hydroxide Nanoplates (M = Co, Ni) Using
- Author
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Eve Y, Martinez, Kuixin, Zhu, and Christina W, Li
- Abstract
Ambipolar doping of metal oxides is critical toward broadening the functionality of semiconducting oxides in electronic devices. Most metal oxides, however, show a strong preference for a single doping polarity due to the intrinsic stability of particular defects in an oxide lattice. In this work, we demonstrate that layered metal hydroxide nanomaterials of Co and Ni, which are intrinsically p-doped in their anhydrous rock salt form, can be n-doped using
- Published
- 2020
16. Systematic Control of Redox Properties and Oxygen Reduction Reactivity through Colloidal Ligand-Exchange Deposition of Pd on Au
- Author
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Christina W. Li, Xueyong Zhang, Xiaoxi Huang, and Alexander J. Shumski
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Chemistry ,Inorganic chemistry ,Oxide ,Nanoparticle ,02 engineering and technology ,General Chemistry ,Overpotential ,engineering.material ,010402 general chemistry ,021001 nanoscience & nanotechnology ,01 natural sciences ,Biochemistry ,Redox ,Catalysis ,0104 chemical sciences ,chemistry.chemical_compound ,Colloid and Surface Chemistry ,Adsorption ,Monolayer ,engineering ,Noble metal ,0210 nano-technology - Abstract
Core-shell nanoparticles of Au@Pd with precise submonolayer, monolayer, or multilayer structure were synthesized using ligand-exchange reactions of palladate ions onto colloidal Au nanocrystals. Decoupling the palladate adsorption step from the subsequent reduction enables excellent precision, uniformity, and tunability in the Pd shell thickness. The redox properties of the surface Pd are directly correlated to the thickness of the Pd shell with a+200 mV shift in the PdO reduction potential for submonolayer Au@Pd nanoparticles compared to pure Pd. Using these precisely controlled core-shell materials, the oxygen reduction catalytic activity can be directly correlated to PdO reduction potential and Pd surface coverage on Au. When the Pd oxide reduction peak is shifted by +240 mV compared to pure Pd, a 50 mV reduction in overpotential and a 4-fold increase in kinetic current density for oxygen reduction are observed. Colloidal ligand-exchange synthesis may be particularly useful for noble metal core-shell catalysts as a strategy to subtly tune the electronic properties of surface atoms in order to lower overpotential and increase catalytic turnover.
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- 2018
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17. The Local Ultraviolet to Infrared Treasury. I. Survey Overview of the Broadband Imaging
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Karoline M. Gilbert, Yumi Choi, Martha L. Boyer, Benjamin F. Williams, Daniel R. Weisz, Eric F. Bell, Julianne J. Dalcanton, Kristen B. W. McQuinn, Evan D. Skillman, Guglielmo Costa, Andrew E. Dolphin, Morgan Fouesneau, Léo Girardi, Steven R. Goldman, Karl D. Gordon, Puragra Guhathakurta, Maude Gull, Lea Hagen, Ky Huynh, Christina W. Lindberg, Paola Marigo, Claire E. Murray, Giada Pastorelli, and Petia Yanchulova Merica-Jones
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Stellar populations ,Dwarf irregular galaxies ,Multi-color photometry ,Astrophysics ,QB460-466 - Abstract
The Local Ultraviolet to Infrared Treasury (LUVIT) is a Hubble Space Telescope program that combines newly acquired data in the near-ultraviolet (NUV), optical, and near-infrared (NIR) with archival optical and NIR imaging to produce multiband panchromatic resolved stellar catalogs for 23 pointings in 22 low-mass, star-forming galaxies ranging in distance from the outskirts of the Local Group to ∼3.8 Mpc. We describe the survey design, detail the LUVIT broadband filter observations and the archival data sets included in the LUVIT reductions, and summarize the simultaneous multiband data reduction steps. The spatial distributions and color–magnitude diagrams (CMDs) from the resulting stellar catalogs are presented for each target, from the NUV to the NIR. We demonstrate in which regions of the CMDs stars with NUV and optical, optical and NIR, and NUV through NIR detections reside. For each target, we use the results from artificial star tests to measure representative completeness, bias, and total photometric uncertainty as a function of magnitude in each broadband filter. We also assess which LUVIT targets have significant spatial variation in the fraction of stars recovered at a given magnitude. The panchromatic LUVIT stellar catalogs will provide a rich legacy data set for a host of resolved stellar population studies.
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- 2024
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18. The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). VI. The High-mass Stellar Initial Mass Function of M33
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Tobin M. Wainer, Benjamin F. Williams, L. Clifton Johnson, Daniel R. Weisz, Julianne J. Dalcanton, Anil C. Seth, Andrew Dolphin, Meredith J. Durbin, Eric F. Bell, Zhuo Chen, Puragra Guhathakurta, Eric W. Koch, Christina W. Lindberg, Erik Rosolowsky, Karin M. Sandstrom, Evan D. Skillman, Adam Smercina, and Estephani E. TorresVillanueva
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Star clusters ,Star formation ,Triangulum Galaxy ,Local Group ,Initial mass function ,Stellar mass functions ,Astronomy ,QB1-991 - Abstract
We measure the high-mass stellar initial mass function (IMF) from resolved stars in M33 young stellar clusters. Leveraging the Hubble Space Telescope’s high resolving power, we fully model the IMF probabilistically. We first model the optical color–magnitude diagram of each cluster to constrain its power-law slope Γ, marginalized over other cluster parameters in the fit (e.g., cluster age, mass, and radius). We then probabilistically model the distribution of mass function (MF) slopes for a highly strict cluster sample of nine clusters more massive than log(Mass/ M _⊙ ) = 3.6; above this mass, all clusters have well-populated main sequences of massive stars and should have accurate recovery of their MF slopes, based on extensive tests with artificial clusters. We find that the ensemble IMF is best described by a mean high-mass slope of $\overline{{\rm{\Gamma }}}=1.49\pm 0.18$ , with an intrinsic scatter of ${\sigma }_{{\rm{\Gamma }}}^{2}={0.02}_{0.00}^{+0.16}$ , consistent with a universal IMF. We find no dependence of the IMF on environmental impacts such as the local star formation rate (SFR) or galactocentric radius within M33, which serves as a proxy for metallicity. This $\overline{{\rm{\Gamma }}}$ measurement is consistent with similar measurements in M31, despite M33 having a much higher SFR intensity. While this measurement is formally consistent with the canonical Kroupa (Γ = 1.30) IMF, as well as the Salpeter (Γ = 1.35) value, it is the second Local Group cluster sample to show evidence for a somewhat steeper high-mass IMF slope. We explore the impacts a steeper IMF slope has on a number of astronomical subfields.
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- 2024
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19. Scylla. III. The Outside-in Radial Age Gradient in the Small Magellanic Cloud and the Star Formation Histories of the Main Body, Wing, and Outer Regions
- Author
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Roger E. Cohen, Kristen B. W. McQuinn, Claire E. Murray, Benjamin F. Williams, Yumi Choi, Christina W. Lindberg, Clare Burhenne, Karl D. Gordon, Petia Yanchulova Merica-Jones, Caroline Bot, Andrew E. Dolphin, Karoline M. Gilbert, Steven Goldman, Alec S. Hirschauer, Karin M. Sandstrom, and O. Grace Telford
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Magellanic Clouds ,Small Magellanic Cloud ,Galaxy evolution ,Local Group ,Astrophysics ,QB460-466 - Abstract
The proximity of the Large and Small Magellanic Clouds (LMC and SMC) provides the opportunity to study the impact of dwarf–dwarf interactions on their mass assembly with a unique level of detail. To this end, we analyze two-filter broadband imaging of 83 Hubble Space Telescope (HST) pointings covering 0.203 deg ^2 toward the SMC, extending out to ∼3.5 kpc in projection from its optical center. Lifetime star formation histories (SFHs) fit to each pointing independently reveal an outside-in age gradient such that fields in the SMC outskirts are older on average. We measure radial gradients of the look-back time to form 90%, 75%, and 50% of the cumulative stellar mass for the first time, finding δ ( τ _90 , τ _75 , τ _50 )/ δ R = (0.61 ${}_{-0.07}^{+0.08}$ , ${0.65}_{-0.08}^{+0.09}$ , ${0.82}_{-0.16}^{+0.12}$ ) Gyr kpc ^−1 assuming PARSEC evolutionary models and a commonly used elliptical geometry of the SMC, although our results are robust to these assumptions. The wing of the SMC deviates from this trend, forming 25% of its cumulative mass over the most recent 3 Gyr owing to a best-fit star formation rate that remains approximately constant. Our results are consistent with chemodynamical evidence of a tidally stripped SMC component in the foreground and imply contributions to the observed SFH from multiple previous LMC–SMC interactions. We also compare our SMC SFH with results from a companion study of the LMC, finding that while the two galaxies present different internal, spatially resolved SFH trends, both the LMC and SMC have similar near-constant lifetime SFHs when viewed globally.
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- 2024
- Full Text
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20. Scylla. II. The Spatially Resolved Star Formation History of the Large Magellanic Cloud Reveals an Inverted Radial Age Gradient
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Roger E. Cohen, Kristen B. W. McQuinn, Claire E. Murray, Benjamin F. Williams, Yumi Choi, Christina W. Lindberg, Clare Burhenne, Karl D. Gordon, Petia Yanchulova Merica-Jones, Karoline M. Gilbert, Martha L. Boyer, Steven Goldman, Andrew E. Dolphin, and O. Grace Telford
- Subjects
Local Group ,Magellanic Clouds ,Galaxy evolution ,Astrophysics ,QB460-466 - Abstract
The proximity of the Magellanic Clouds provides the opportunity to study interacting dwarf galaxies near a massive host, and spatial trends in their stellar population properties in particular, with a unique level of detail. The Scylla pure parallel program has obtained deep (80% complete to >1 mag below the ancient main-sequence turnoff), homogeneous two-filter Hubble Space Telescope imaging sampling the inner star-forming disk of the Large Magellanic Cloud (LMC), the perfect complement to shallower, contiguous ground-based surveys. We harness this imaging together with extant archival data and fit lifetime star formation histories (SFHs) to resolved color–magnitude diagrams of 111 individual fields, using three different stellar evolutionary libraries. We validate per-field recovered distances and extinctions, as well as the combined global LMC age–metallicity relation and SFH against independent estimates. We find that the present-day radial age gradient reverses from an inside-out gradient in the inner disk to an outside-in gradient beyond ∼2 disk scale lengths, supported by ground-based measurements. The gradients become relatively flatter at earlier look-back times, while the location of the inversion remains constant over an order of magnitude in look-back time, from ∼1 to 10 Gyr. This suggests at least one mechanism that predates the recent intense LMC–Small Magellanic Cloud interaction. We compare observed radial age trends to other late-type galaxies at fixed stellar mass and discuss similarities and differences in the context of potential drivers, implying strong radial migration in the LMC.
- Published
- 2024
- Full Text
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21. Scylla. I. A Pure-parallel, Multiwavelength Imaging Survey of the ULLYSES Fields in the LMC and SMC
- Author
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Claire E. Murray, Christina W. Lindberg, Petia Yanchulova Merica-Jones, Benjamin F. Williams, Roger E. Cohen, Karl D. Gordon, Kristen B. W. McQuinn, Yumi Choi, Clare Burhenne, Karin M. Sandstrom, Caroline Bot, L. Clifton Johnson, Steven R. Goldman, Christopher J. R. Clark, Julia C. Roman-Duval, Karoline M. Gilbert, J. E. G. Peek, Alec S. Hirschauer, Martha L. Boyer, and Andrew E. Dolphin
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Magellanic Clouds ,Hubble Space Telescope ,Surveys ,Catalogs ,Star formation ,Interstellar medium ,Astrophysics ,QB460-466 - Abstract
Scylla is a deep Hubble Space Telescope (HST) survey of the stellar populations, interstellar medium, and star formation in the LMC and SMC. As a pure-parallel complement to the Ultraviolet Legacy Library of Young Stars as Essential Standards (ULLYSES) survey, Scylla obtained 342 orbits of ultraviolet (UV) through near-IR imaging of the LMC and SMC with Wide Field Camera 3. In this paper, we describe the science objectives, observing strategy, data reduction procedure, and initial results from our photometric analysis of 96 observed fields. Although our observations were constrained by ULLYSES primary exposures, we imaged all fields in at least two filters (F475W and F814W) and 64% of fields in at least three and as many as seven WFC3 filters spanning the UV to IR. Overall, we reach average 50% completeness of m _F225W = 26.0, m _F275W = 26.2, m _F336W = 26.9, m _F475W = 27.8, m _F814W = 25.5, m _F110W = 24.7, and m _F160W = 24.0 Vega mag in our photometric catalogs, which is faintward of the ancient main-sequence turnoff in all filters. The primary science goals of Scylla include characterizing the structure and properties of dust in the MCs, as well as their spatially resolved star formation and chemical enrichment histories. Our images and photometric catalogs, which represent the widest-area coverage of MCs with HST photometry to date, are available as a high-level science product at the Barbara A. Mikulski Archive for Space Telescopes.
- Published
- 2024
- Full Text
- View/download PDF
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