"Dead Quasars" in Nearby Galaxies?
- 16 February 1990
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 247 (4944) , 817-823
- https://doi.org/10.1126/science.247.4944.817
Abstract
The nuclei of some galaxies undergo violent activity, quasars being the most extreme instances of this phenomenon. Such activity is probably short-lived compared to galactic lifetimes, and was most prevalent when the universe was only about one-fifth of its present age. A massive black hole seems the inevitable end point of such activity, and dead quasars should greatly outnumber active ones. In recent years, studies of stellar motions in the cores of several nearby galaxies indicate the presence of central dark masses which could be black holes. This article discusses how such evidence might be corroborated, and the potential implications for our understanding of active galaxies and black holes.Keywords
This publication has 40 references indexed in Scilit:
- Eddington ratios as a constraint on the activity patterns of the active galactic nucleiThe Astrophysical Journal, 1988
- Evidence for a supermassive black hole in the nucleus of M31The Astrophysical Journal, 1988
- Stellar dynamics in the nuclei of M31 and M32 - Evidence for massive black holes?The Astrophysical Journal, 1988
- A central black hole in M32The Astrophysical Journal, 1987
- The Galactic Center: Is It a Massive Black Hole?Science, 1986
- Studying the internal kinematics of galaxies using the calcium infrared tripletThe Astrophysical Journal, 1984
- Evidence for a central mass concentration in M32The Astrophysical Journal, 1984
- The passage of a star by a massive black holeThe Astrophysical Journal, 1982
- The nature of the central parsec of the GalaxyThe Astrophysical Journal, 1982
- Possible power source of Seyfert galaxies and QSOsNature, 1975