On the Superluminal Motion of Radio-Loud AGNs
Apparent superluminal motion of different radio-loud AGNs are similarly related with beaming effect. The cosmological expanding effect would play no part in the superluminal motion of radio galaxies, BL Lacertae objects as well as quasars. Meanwhile, we confirm that estimates for apparent velocity βapp and Doppler boosting factor S based on multi-wavelength combination and variability are comparable.
Zhi-BinZhang Yi-Zhen Zhang
College of Science,Guizhou University,Guiyang,Guizhou 550025,China The Joint Research Center for Astronomy Sponsored by GZU and NAOC,Guiyang,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
247-249
2010-09-20(万方平台首次上网日期,不代表论文的发表时间)