{ "id": "astro-ph/0007369", "version": "v1", "published": "2000-07-25T11:54:56.000Z", "updated": "2000-07-25T11:54:56.000Z", "title": "The correlation between black hole mass and bulge velocity dispersion in hierarchical galaxy formation models", "authors": [ "Martin G. Haehnelt", "Guinevere Kauffmann" ], "comment": "5 pages, LaTeX, 3 postscript figures included; submitted to MNRAS", "journal": "Mon.Not.Roy.Astron.Soc. 318 (2000) L35", "doi": "10.1046/j.1365-8711.2000.03989.x", "categories": [ "astro-ph" ], "abstract": "Recent work has demonstrated that there is a tight correlation between the mass of a black hole and the velocity dispersion of the bulge of its host galaxy. We show that the model of Kauffmann & Haehnelt, in which bulges and supermassive black holes both form during major mergers, produces a correlation between M_bh and sigma with slope and scatter comparable to the observed relation. In the model, the M_bh - sigma relation is significantly tighter than the correlation between black hole mass and bulge luminosity or the correlation between bulge luminosity and velocity dispersion. There are two reasons for this: i) the gas masses of bulge progenitors depend on the velocity dispersion but not on the formation epoch of the bulge, whereas the stellar masses of the progenitors depend on both; ii) mergers between galaxies move black holes along the observed M_bh - sigma relation, even at late times when the galaxies are gas-poor and black holes grow mainly by merging of pre-existing black holes. We conclude that the small scatter in the observed M_bh - sigma relation is consistent with a picture in which bulges and black holes form over a wide range in redshift.", "revisions": [ { "version": "v1", "updated": "2000-07-25T11:54:56.000Z" } ], "analyses": { "keywords": [ "black hole mass", "hierarchical galaxy formation models", "bulge velocity dispersion", "correlation", "sigma relation" ], "tags": [ "journal article" ], "note": { "typesetting": "LaTeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 546821 } } }