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
Gespeichert in:
| Hauptverfasser: | , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
29 January 2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 476, Heft: 1, Pages: 366-380 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty208 |
| Online-Zugang: | 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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| Verfasserangaben: | T. C. N. Boekholt, D. R. G. Schleicher, M. Fellhauer, R. S. Klessen, B. Reinoso, A. M. Stutz, L. Haemmerlé |
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