Tracing the relation between black holes and dark haloes
| dc.creator | Buyle, Pieter | |
| dc.creator | Baes, Maarten | |
| dc.creator | Dejonghe, Herwig | |
| dc.date | 2003-11-26 | |
| dc.date.accessioned | 2026-07-07T02:11:21Z | |
| dc.date.available | 2026-07-07T02:11:21Z | |
| dc.description | We present new velocity dispersion measurements for a set of 12 spiral galaxies and use them to derive a more accurate V_c - sigma relation which holds for a wide morphological range of galaxies. Combined with the M_BH - sigma relation, this relation can be used as a tool to estimate supermassive black hole (SMBH) masses by means of the asymptotic circular velocity. Together with the Tully-Fisher relation, it serves as a constraint for galaxy formation and evolution models. | |
| dc.description | 2 pages, 2 figures, to appear in Proc. IAU Symp. 220, "Dark Matter in Galaxies" eds. S. Ryder, D.J. Pisano, M. Walker, & K. Freeman (San Francisco: ASP) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0311579 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0311579 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7050 | |
| dc.subject | Astrophysics | |
| dc.title | Tracing the relation between black holes and dark haloes | |
| dc.type | text |