The evolution of supermassive Population III stars
Abstract. Supermassive primordial stars forming in atomically cooled haloes at z ∼ 15-20 are currently thought to be the progenitors of the earliest quasars in
Gespeichert in:
| Hauptverfasser: | , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 474, Heft: 2, Pages: 2757-2773 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx2919 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1093/mnras/stx2919 Verlag, Volltext: https://academic.oup.com/mnras/article/474/2/2757/4636552 |
| Verfasserangaben: | Lionel Haemmerlé, T.E. Woods, Ralf S. Klessen, Alexander Heger, Daniel J. Whalen |
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