On the masses of black holes in radio-loud quasars

被引：109

作者：

Gu, MF ^{[1
]}

Cao, XW

Jiang, DR

机构：

[1] Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China

[2] Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2001年 / 327卷 / 04期

关键词：

galaxies : active; galaxies : nuclei; quasars : general;

D O I：

10.1046/j.1365-8711.2001.04795.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The central black hole masses of a sample of radio-loud quasars are estimated by using the data of H beta linewidth and the optical continuum luminosity. The vast majority of the quasars in this sample have black hole masses larger than 10(8) M-circle dot, while a few quasars may contain relatively smaller black holes. We found a significant anti-correlation between the radio loudness and the central black hole mass. It might imply that the jet formation is governed by the black hole mass.

引用

页码：1111 / 1115

页数：5

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