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821
Terrestrial- and Neptune-mass Free-Floating Planet Candidates from the MOA-II 9 yr Galactic Bulge Survey
Published 2023-01-01“…This allows us to use a Galactic model to simulate the t _E and θ _E distribution of events produced by the known stellar populations and models of the FFP distribution that are fit to the data. …”
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822
GOALS-JWST: NIRCam and MIRI Imaging of the Circumnuclear Starburst Ring in NGC 7469
Published 2023-01-01“…Their NIR colors are also consistent with young (<5 Myr) stellar populations and more than half of them are coincident with the mid-infrared (MIR) emission peaks. …”
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823
THE CHEMICAL EVOLUTION OF THE BOÖTES I ULTRA-FAINT DWARF GALAXY
Published 2018“…This resulted in the two stellar populations observable today.…”
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824
Unusual Isotopic Abundances in a Fully Convective Stellar Binary
Published 2019“…These isotopic measurements complement the elemental abundances provided by large-scale spectroscopic surveys, and open a new window onto studies of Galactic evolution, stellar populations, and individual systems. Key words: infrared: stars – techniques: spectroscopic – stars: abundances – supernovae: general…”
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825
Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
Published 2022“…Galaxy morphologies, kinematics, and stellar populations are thought to be linked to each other. …”
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826
ChAInGeS: THE CHANDRA ARP INTERACTING GALAXIES SURVEY
Published 2015“…However, the u – g and r – i colors at the ULX locations tend to be bluer on average than these global colors, suggesting that ULXs are preferentially found in regions with young stellar populations. In the Arp sample there is a possible enhancement of a factor of ~2-5 in the fraction of galactic nuclei that are X-ray-bright compared to more normal spirals.…”
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827
First JWST Observations of JAGB Stars in the SN Ia Host Galaxies: NGC 7250, NGC 4536, NGC 3972
Published 2024-01-01“…After successfully employing this method in our JWST galaxy sample, we find the JAGB stars are well segregated from other stellar populations in color–magnitude space, and have observed dispersions about their individual F115W modes of σ _N7250 = 0.32 mag, σ _N4536 = 0.34 mag, and σ _N3972 = 0.35 mag. …”
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828
Probing the Star Formation Main Sequence Down to 108 M ⊙ at 1.0 < z < 3.0
Published 2023-01-01“…These observational characteristics are identified with young (mass-weighted age 〈 t _M _− _w 〉 ∼ 0.014 Gyr) stellar populations subject to low attenuations (〈 A ( V )〉 ∼ 0.30 mag). …”
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829
Exposing Line Emission: The Systematic Differences of Measuring Galaxy Stellar Masses with JWST NIRCam Medium versus Wide Band Photometry
Published 2024-01-01“…There are, however, a subset of galaxies (5% at z ∼ 2 up to 15% at z ∼ 6) where wide bands underestimate emission line strengths and infer older stellar populations, leading to median stellar mass differences of ∼0.7 dex. …”
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830
Optical- and UV-continuum Morphologies of Compact Radio Source Hosts
Published 2024-01-01“…Young (≲ 10 Myr), massive (≳ 5 M _⊙ ) stellar populations are likely to be the dominant source of the blue excess emission in radio galaxies at these redshifts. …”
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831
Scylla. I. A Pure-parallel, Multiwavelength Imaging Survey of the ULLYSES Fields in the LMC and SMC
Published 2024-01-01“…Scylla is a deep Hubble Space Telescope (HST) survey of the stellar populations, interstellar medium, and star formation in the LMC and SMC. …”
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832
PHANGS-ML: Dissecting Multiphase Gas and Dust in Nearby Galaxies Using Machine Learning
Published 2024-01-01“…We focus on three of the PHANGS-JWST galaxies, for which we extract properties pertaining to their stellar populations; warm ionized and cold molecular gas; and polycyclic aromatic hydrocarbons (PAHs), as measured over 150 pc scale regions. …”
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833
An Empirical Framework Characterizing the Metallicity and Star-formation History Dependence of X-Ray Binary Population Formation and Emission in Galaxies
Published 2024-01-01“…Integration of our models provides predictions for X-ray scaling relations that agree very well with past results presented in the literature, including, e.g., the L _X –SFR– Z relation for high-mass XRBs in young stellar populations as well as the L _X / M _⋆ ratio observed in early-type galaxies that harbor old populations of low-mass XRBs. …”
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834
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy [version 2; peer review: 2 approved]
Published 2025-02-01“…The complex interactions of those gas, dust and stellar populations form what has come to be known as the ecology of our Galaxy. …”
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835
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy [version 1; peer review: 2 approved]
Published 2024-06-01“…The complex interactions of those gas, dust and stellar populations form what has come to be known as the ecology of our Galaxy. …”
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836
Observations of Extremely Metal-poor O Stars: Weak Winds and Constraints for Evolution Models
Published 2024-01-01“…These results provide empirical benchmarks for future development of mass-loss and evolution models for metal-poor stellar populations.…”
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837
Small Region, Big Impact: Highly Anisotropic Lyman-continuum Escape from a Compact Starburst Region with Extreme Physical Properties
Published 2023-01-01“…Extreme, young stellar populations are considered to be the primary contributor to cosmic reionization. …”
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838
Radial Profiles of Σ*, ΣSFR, Gas Metallicity, and Their Correlations across the Galactic Mass–Size Plane
Published 2024-01-01“…The combination of higher sSFR and potentially higher star formation efficiency in compact galaxies suggests that their central gas is being rapidly consumed, leading to older stellar populations, as indicated by D _n (4000) and EW(H δ _A ), and resulting in faster central growth. …”
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839
A JWST Survey of the Supernova Remnant Cassiopeia A
Published 2024-01-01“…These JWST survey data and initial findings help address unresolved questions about massive star explosions that have broad implications for the formation and evolution of stellar populations, the metal and dust enrichment of galaxies, and the origin of compact remnant objects.…”
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840
The Comprehensive Archive of Substellar and Planetary Accretion Rates
Published 2023-01-01“…However, we argue that the brown-dwarf and stellar populations are better described separately and by accounting for both mass and age. …”
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