Showing 821 - 840 results of 878 for search '"stellar population"', query time: 0.52s Refine Results
  1. 821
  2. 822
  3. 823
  4. 824

    Unusual Isotopic Abundances in a Fully Convective Stellar Binary by Lothringer, J. D., Flores, B., Mills, E. A. C., Freedman, R., Valverde, J., Miles, B., Skemer, A., Crossfield, Ian Jm, Guo, Xueying

    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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    Article
  5. 825
  6. 826

    ChAInGeS: THE CHANDRA ARP INTERACTING GALAXIES SURVEY by Smith, Beverly J., Swartz, Douglas A., Miller, Olivia, Burleson, Jacob A., Nowak, Michael A., Struck, Curtis

    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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    Article
  7. 827

    First JWST Observations of JAGB Stars in the SN Ia Host Galaxies: NGC 7250, NGC 4536, NGC 3972 by Abigail J. Lee, Wendy L. Freedman, In Sung Jang, Barry F. Madore, Kayla A. Owens

    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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    Article
  8. 828

    Probing the Star Formation Main Sequence Down to 108 M ⊙ at 1.0 < z < 3.0 by Rosa M. Mérida, Pablo G. Pérez-González, Patricia Sánchez-Blázquez, Ángela García-Argumánez, Marianna Annunziatella, Luca Costantin, Alejandro Lumbreras-Calle, Belén Alcalde-Pampliega, Guillermo Barro, Néstor Espino-Briones, Anton M. Koekemoer

    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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    Article
  9. 829

    Exposing Line Emission: The Systematic Differences of Measuring Galaxy Stellar Masses with JWST NIRCam Medium versus Wide Band Photometry by Ghassan T. E. Sarrouh, Adam Muzzin, Kartheik G. Iyer, Lamiya Mowla, Sunna Withers, Nicholas S. Martis, Roberto Abraham, Yoshihisa Asada, Maruša Bradač, Gabriel B. Brammer, Guillaume Desprez, Vince Estrada-Carpenter, Jasleen Matharu, Gaël Noirot, Marcin Sawicki, Victoria Strait, Chris J. Willott, Johannes Zabl

    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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    Article
  10. 830

    Optical- and UV-continuum Morphologies of Compact Radio Source Hosts by C. Duggal, C. P. O’Dea, S. A. Baum, A. Labiano, C. Tadhunter, D. M. Worrall, R. Morganti, G. R. Tremblay, D. Dicken

    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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    Article
  11. 831
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  13. 833

    An Empirical Framework Characterizing the Metallicity and Star-formation History Dependence of X-Ray Binary Population Formation and Emission in Galaxies by Bret D. Lehmer, Erik B. Monson, Rafael T. Eufrasio, Amirnezam Amiri, Keith Doore, Antara Basu-Zych, Kristen Garofali, Lidia Oskinova, Jeff J. Andrews, Vallia Antoniou, Robel Geda, Jenny E. Greene, Konstantinos Kovlakas, Margaret Lazzarini, Chris T. Richardson

    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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  14. 834
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    Observations of Extremely Metal-poor O Stars: Weak Winds and Constraints for Evolution Models by O. Grace Telford, John Chisholm, Andreas A. C. Sander, Varsha Ramachandran, Kristen B. W. McQuinn, Danielle A. Berg

    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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  17. 837
  18. 838

    Radial Profiles of Σ*, ΣSFR, Gas Metallicity, and Their Correlations across the Galactic Mass–Size Plane by Lin Lin, Shiyin Shen, Hassen M. Yesuf, Ye-Wei Mao, Lei Hao

    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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  19. 839
  20. 840

    The Comprehensive Archive of Substellar and Planetary Accretion Rates by S. K. Betti, K. B. Follette, K. Ward-Duong, A. E. Peck, Y. Aoyama, J. Bary, B. Dacus, S. Edwards, G.-D. Marleau, K. Mohamed, J. Palmo, C. Plunkett, C. Robinson, H. Wang

    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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