other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2013MNRAS.429.2199S - Mon. Not. R. Astron. Soc., 429, 2199-2211 (2013/March-1)
Galaxy zoo: bulgeless galaxies with growing black holes.
SIMMONS B.D., LINTOTT C., SCHAWINSKI K., MORAN E.C., HAN A., KAVIRAJ S., MASTERS K.L., URRY C.M., WILLETT K.W., BAMFORD S.P. and NICHOL R.C.
Abstract (from CDS):
The black hole masses are systematically higher than expected from established bulge-black hole relations. However, if the mean Eddington ratio of the systems with measured black hole masses (L/LEdd ~ 0.065) is typical, 10 of 13 sources are consistent with the correlation between black hole mass and total stellar mass. That pure disc galaxies and their central black holes may be consistent with a relation derived from elliptical and bulge-dominated galaxies with very different formation histories implies the details of stellar galaxy evolution and dynamics may not be fundamental to the co-evolution of galaxies and black holes.
Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)
Journal keyword(s): galaxies: active - galaxies: bulges - galaxies: evolution - galaxies: general - galaxies: Seyfert - galaxies: spiral
Simbad objects: 21
To bookmark this query, right click on this link: simbad:2013MNRAS.429.2199S and select 'bookmark this link' or equivalent in the popup menu