Black hole masses of BL LAC objects

被引：0
|
作者：
Kotilainen, JK [1 ]
Falomo, R [1 ]
Treves, A [1 ]
机构：
[1] Univ Turku, Tuorla Observ, FIN-21500 Piikkio, Finland
来源：
GALAXY EVOLUTION: THEORY AND OBSERVATIONS | 2003年 / 17卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The black hole (BH) mass [M(BH)] is of paramount importance in AGN models, as the dependence of M(BH) on host galaxy properties provides clues to the role of BHs in galaxy formation and evolution. The only direct dynamical method for measuring M(BH) in AGN is the time-consuming reverberation mapping of broad emission lines. Consequently, only for a few AGN M(BH) is known (e.g. Kaspi et al. 2000; Wandel 2002).
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页码：198 / 198
页数：1
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