The chemical signature of surviving Population III stars in the Milky Way
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/453/3/2771/4930593/stv1815.pdf
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1. Simulating the Collapse of Rotating Primordial Gas Clouds to Study the Possibility of the Survival of Population III Protostars;The Astrophysical Journal;2023-02-01
2. Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the JWST;The Astronomical Journal;2022-12-02
3. The impact of carbon and oxygen abundances on the metal-poor initial mass function;Monthly Notices of the Royal Astronomical Society;2022-11-12
4. Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?;Publications of the Astronomical Society of Japan;2022-03-26
5. Modeling the Survival of Population III Stars to the Present Day;The Astrophysical Journal;2020-09-17
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