Investigating the Disk-corona Relation in Radio-quiet and Radio-Ioud AGNs
We compile a blue AGN sample with 240 radio-quiet (RQ) and 18 radio loud (RL) objects. We investigate the dependence of ratio of hard X-ray luminosity to bolometric luminosity on black hole mass and Eddington ratio. We find that the hard X-ray fraction log(L2_lOOkev/Lbol) decreases with the increase of Eddington ratio for RQ AGNs, which is not the case for RL AGNs. We also find that the hard X-ray fraction is independent on black hole mass for both RQ and RL AGNs. The implication is discussed in the end of the poster.
accretion accretion disks - galaxies active - X-rays galaxies
J.Y. Liu B.F. Liu
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences,PO Box 110, Kun National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences,PO Box 110, Kun
国际会议
The 10th Asian-Pacific Regional International Astronomical Union Meeting(第十届亚洲及太平洋地区天文学大会 APRIM)
昆明
英文
239-240
2008-08-03(万方平台首次上网日期,不代表论文的发表时间)