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Formation of massive seed black holes via collisions and accretion

Abstract. Models aiming to explain the formation of massive black hole seeds, and in particular the direct collapse scenario, face substantial difficulties. Th

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Main Authors: Boekholt, Tjarda (Author) , Schleicher, D. R. G. (Author) , Fellhauer, M. (Author) , Klessen, Ralf S. (Author) , Reinoso, B. (Author) , Stutz, A. M. (Author) , Haemmerlé, L. (Author)
Format: Article (Journal)
Language:English
Published: 29 January 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 476, Issue: 1, Pages: 366-380
ISSN:1365-2966
DOI:10.1093/mnras/sty208
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/sty208
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/476/1/366/4828377
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Author Notes:T. C. N. Boekholt, D. R. G. Schleicher, M. Fellhauer, R. S. Klessen, B. Reinoso, A. M. Stutz, L. Haemmerlé
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Summary:Abstract. Models aiming to explain the formation of massive black hole seeds, and in particular the direct collapse scenario, face substantial difficulties. Th
Item Description:Gesehen am 02.04.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty208

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