A Dramatic Decrease in Carbon Star Formation in M31
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab24e2/pdf
Reference74 articles.
1. Synthetic photometry for M and K giants and stellar evolution: hydrostatic dust-free model atmospheres and chemical abundances
2. Synthetic photometry for carbon rich giants
3. Comparison of stellar population model predictions using optical and infrared spectroscopy
4. Dusty Waves on a Starry Sea: The Mid-Infrared View of M31
5. The calibration of the metallicity versus C/M relation
Cited by 20 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Erratum: “A Census of Thermally Pulsing AGB Stars in the Andromeda Galaxy and a First Estimate of their Contribution to the Global Dust Budget” (2022, ApJS, 259, 41);The Astrophysical Journal Supplement Series;2023-10-01
2. Carbon Stars as Standard Candles: An Empirical Test for the Reddening, Metallicity, and Age Sensitivity of the J-region Asymptotic Giant Branch (JAGB) Method;The Astrophysical Journal;2023-10-01
3. Hubble Space Telescope imaging of the compact elliptical galaxy M32 reveals a dearth of carbon stars;Monthly Notices of the Royal Astronomical Society;2023-08-25
4. The JWST Resolved Stellar Populations Early Release Science Program. II. Survey Overview;The Astrophysical Journal Supplement Series;2023-08-24
5. A Census of Thermally Pulsing AGB Stars in the Andromeda Galaxy and a First Estimate of Their Contribution to the Global Dust Budget;The Astrophysical Journal Supplement Series;2022-03-23
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