Did supermassive black holes form by direct collapse?

dc.creatorBegelman, Mitchell C.
dc.date2007-09-04
dc.date.accessioned2026-07-07T11:19:05Z
dc.date.available2026-07-07T11:19:05Z
dc.descriptionRapid infall of gas in the nuclei of galaxies could lead to the formation of black holes by direct collapse, without first forming stars. Black holes formed in this way would have initial masses of a few solar masses, but would be embedded in massive envelopes that would allow them to grow at a highly super-Eddington rate. Thus, seed black holes as large as 10^3-10^4 solar masses could form very rapidly. I will sketch the basic physics of the direct collapse process and the properties of the accreting envelopes.
dc.description5 pages, 2 figures. To appear in "First Stars III", proceedings of the conference in Santa Fe, NM, July 16-20, 2007, eds. B. O'Shea, A. Heger and T. Abel. AIP Conference Proceedings
dc.identifierhttps://arxiv.org/abs/0709.0545
dc.identifierhttp://arxiv.org/abs/0709.0545
dc.identifierAIPConf.Proc.990:489-493,2008
dc.identifierdoi:10.1063/1.2905669
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193566
dc.subjectAstrophysics
dc.titleDid supermassive black holes form by direct collapse?
dc.typetext

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