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Spin evolution and feedback of supermassive black holes in cosmological simulations

ABSTRACT. It is well established that the properties of supermassive black holes (BHs) and their host galaxies are correlated through scaling relations. While

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Bibliographic Details
Main Authors: Bustamente, Sebastian (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 14 October 2019
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 490, Issue: 3, Pages: 4133-4153
ISSN:1365-2966
DOI:10.1093/mnras/stz2836
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stz2836
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/490/3/4133/5586997
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Author Notes:Sebastian Bustamante, Volker Springel
Description
Summary:ABSTRACT. It is well established that the properties of supermassive black holes (BHs) and their host galaxies are correlated through scaling relations. While
Item Description:Gesehen am 06.03.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz2836

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