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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

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Bibliographic Details
Main Authors: Haemmerlé, Lionel (Author) , Woods, Tyrone E. (Author) , Klessen, Ralf S. (Author) , Heger, Alexander (Author) , Whalen, Daniel J. (Author)
Format: Article (Journal)
Language:English
Published: 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 474, Issue: 2, Pages: 2757-2773
ISSN:1365-2966
DOI:10.1093/mnras/stx2919
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/stx2919
Verlag, Volltext: https://academic.oup.com/mnras/article/474/2/2757/4636552
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Author Notes:Lionel Haemmerlé, T.E. Woods, Ralf S. Klessen, Alexander Heger, Daniel J. Whalen
Description
Summary: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
Item Description:Published: 16 November 2017
Gesehen am 19.08.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stx2919

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