会议专题

Measurement of Black Hole Mass Radio-Loud Quasars

In this work, we construct a sample of 1585 radioloud quasars to measure their black hole masses using broad emission lines. We compare our black hole masses with the virial black hole masses measured by Shen et al. (2010). We find that there is a large deviation between them if our black hole mass is measured from the CIV broad emission line. Whereas, if our black hole mass is measured from broad emission line of Mg Ⅱ or Hβ, both the values are consistent.

Cheng-YueSu Z.-F.Chen R.-L.He C.-H.Zhang T.-T.Wang

Guangdong University of Technology,Guangzhou 510006,Peoples Republic of China Center for Astrophysics,Guangzhou University,Guangzhou 510006,Peoples Republic of China

国际会议

International Conference of Multiwavelength Variability of Blazars(Blazar多波段光变国际学术会议)

广州

英文

315-317

2010-09-20(万方平台首次上网日期,不代表论文的发表时间)