Black hole mass and accretion rate of Active Galactic Nuclei.pdf
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Black hole mass and accretion rate of Active Galactic Nuclei
Xue-Bing Wu, F.K. Liu, R. Wang
Department of Astronomy, Peking University, Beijing 100871, China
M.Z. Kong, J.L. Han
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
(Received February 28 2006)
The determination of the central black hole mass is crucial to the understanding of AGN physics.
In this paper we briefly review some methods that are currently used to estimate the black hole
mass of AGNs. Particularly we demonstrate the importance of two correlations: one between the
black hole mass and the stellar velocity dispersion and another one between the broad line region
size and the optical continuum luminosity. Besides applying these relations in deriving black hole
masses of various types of AGNs, we also employed the fundamental plane of elliptical galaxies to
estimate the central velocity dispersions of AGN host galaxies, and then the black hole masses of
AGNs including BL Lac objects. In addition, we derived another empirical relation between the
BLR size and Hβ emission line luminosity from AGNs with the BLR size measured by reverberation
mapping studies, and argued that more accurate black hole masses of extremely radio-loud AGNs
could be obtained with it than using the usual R?L
5100A?
relation because of the jet contribution to
the optical continuum. Finally we pointed out that black hole mass estimation is very much helpful
to determine the accretion rate and understand the accretion process in AGNs.
PACS numbers: 04.70.-s; 97.60.Lf; 98.54.Aj; 98.54.Cm
Keywords: Black holes, Quasars; Active Galactic Nuclei
I. INTRODUCTION
As we know, mass is the most important physics pa-
rameter of a black hole. Many other properties of the
black hole are directly related to its mass. Currently
astrophysical black holes can be divided into three cat-
egories: the primordial black holes with the mass of
a
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