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
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
14 October 2019
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2019, Jahrgang: 490, Heft: 3, Pages: 4133-4153 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz2836 |
| Online-Zugang: | 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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| Verfasserangaben: | Sebastian Bustamante, Volker Springel |
| Zusammenfassung: | 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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| Beschreibung: | Gesehen am 06.03.2020 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz2836 |