other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2012MNRAS.422.1586G - Mon. Not. R. Astron. Soc., 422, 1586-1591 (2012/May-2)
Extending the mbh-σ diagram with dense nuclear star clusters.
GRAHAM A.W.
Abstract (from CDS):
Finally, it is predicted that host galaxies fainter than MB ∼ -20.5 mag (i.e. those not formed in dry merger events) which follow the relation Mbh∝σ5, and are thus not `pseudo-bulges', should not have a constant Mbh/Mhost ratio but instead have {img}. It is argued that the previous near-linear {img} and {img} relations have been biased by the sample selection of luminous galaxies, and as such should not be used to constrain the co-evolution of supermassive black holes in galaxies other than those luminous few built by major dry merger events.
Abstract Copyright: 2012 The Author Monthly Notices of the Royal Astronomical Society2012 RAS
Journal keyword(s): galaxies: dwarf - galaxies: fundamental parameters - galaxies: kinematics and dynamics - galaxies: nuclei - galaxies: star clusters: general - galaxies: structure
Simbad objects: 31
To bookmark this query, right click on this link: simbad:2012MNRAS.422.1586G and select 'bookmark this link' or equivalent in the popup menu