Descendants of the first stars: the distinct chemical signature of second-generation stars
ABSTRACT. Extremely metal-poor (EMP) stars in the Milky Way (MW) allow us to infer the properties of their progenitors by comparing their chemical composition
Gespeichert in:
| Hauptverfasser: | , , , , , , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
07 May 2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 478, Heft: 2, Pages: 1795-1810 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1176 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1093/mnras/sty1176 Verlag: https://academic.oup.com/mnras/article/478/2/1795/4993535 
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| Verfasserangaben: | Tilman Hartwig, Naoki Yoshida, Mattis Magg, Anna Frebel, Simon C. O. Glover, Facundo A. Gómez, Brendan Griffen, Miho N. Ishigaki, Alexander P. Ji, Ralf S. Klessen, Brian W. O’Shea, and Nozomu Tominaga |
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