| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1771955 | Chinese Astronomy and Astrophysics | 2008 | 9 Pages |
Abstract
The redshift, central black hole mass and accretion rate are important parameters when studying the AGN evolution. The central black hole masses for 172 quasars and Seyfert galaxies are calculated in this paper using the reverberation mapping method. The distributions of central black hole masses, redshifts and the Eddington accretion rates are analyzed, to verify the transition from the quasar to the Seyfert galaxy in the course of evolution.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Bao Yu-Ying, Zhang Xiong, Chen Luo-En, Zhang Hao-Jing, Peng Zhao-Yang, Zheng Yong-Gang,