Evolution of active galaxies: black-hole mass–bulge relations for narrow line objects
- 31 August 2001
- journal article
- Published by Elsevier BV in New Astronomy
- Vol. 6 (5), 321-329
- https://doi.org/10.1016/s1384-1076(01)00058-6
Abstract
No abstract availableKeywords
This publication has 36 references indexed in Scilit:
- The correlation between black hole mass and bulge velocity dispersion in hierarchical galaxy formation modelsMonthly Notices of the Royal Astronomical Society, 2000
- A Fundamental Relation between Supermassive Black Holes and Their Host GalaxiesThe Astrophysical Journal, 2000
- On the relationship between galaxy formation and quasar evolutionMonthly Notices of the Royal Astronomical Society, 1999
- The obscured growth of massive black holesMonthly Notices of the Royal Astronomical Society, 1999
- High-redshift galaxies, their active nuclei and central black holesMonthly Notices of the Royal Astronomical Society, 1998
- ASCA observations of two steep soft X-ray quasarsMonthly Notices of the Royal Astronomical Society, 1998
- Hubble Space TelescopeImages of a Sample of 20 Nearby Luminous QuasarsThe Astrophysical Journal, 1997
- The Complex Optical to Soft X-Ray Spectrum of Low-Redshift Radio-quiet Quasars. II. Comparison with Free-Free and Accretion Disk ModelsThe Astrophysical Journal, 1995
- A statistical study of properties of Seyfert and starburst galaxiesThe Astrophysical Journal Supplement Series, 1988
- Profiles of emission lines in AGN – I. Observations of [O III] linesMonthly Notices of the Royal Astronomical Society, 1988