Rotation and internal structure of Population III protostars

We analyse the cosmological simulations performed in the recent work of Greif et al., which followed the early growth and merger history of Population III (Pop III) stars while resolving scales as small as 0.05 R⊙. This is the first set of cosmological simulations to self-consistently resolve the ro...

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Bibliographic Details
Main Authors: Stacy, Athena (Author) , Greif, Thomas H. (Author) , Klessen, Ralf S. (Author) , Bromm, Volker (Author) , Loeb, Abraham (Author)
Format: Article (Journal)
Language:English
Published: 2013
In: Monthly notices of the Royal Astronomical Society
Year: 2013, Volume: 431, Issue: 2, Pages: 1470-1486
ISSN:1365-2966
DOI:10.1093/mnras/stt264
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stt264
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/431/2/1470/1455450
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Author Notes:Athena Stacy, Thomas H. Greif, Ralf S. Klessen, Volker Bromm and Abraham Loeb
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