Correlations of the IR luminosity and Eddington ratio with a hard X-ray-selected sample of active galactic nuclei

被引:26
作者
Mushotzy, Richard F. [1 ]
Winter, Lisa M. [2 ]
McIntosh, Daniel H. [3 ]
Tueller, Jack [1 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Univ Maryland, College Pk, MD 20742 USA
[3] Univ Massachusetts, Amherst, MA 01003 USA
来源
ASTROPHYSICAL JOURNAL LETTERS | 2008年 / 684卷 / 02期
基金
美国国家航空航天局;
关键词
galaxies : Seyfert; surveys; X-rays : galaxies;
D O I
10.1086/592196
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use the Swift Burst Alert Telescope (BAT) sample of hard X-ray-selected active galactic nuclei (AGN) with a median redshift of 0.03 and the 2MASS J- and K-band photometry to examine the correlation of hard X-ray emission to Eddington ratio as well as the relationship of the J- and K-band nuclear luminosity to the hard X-ray luminosity. The BAT sample is almost unbiased by the effects of obscuration and thus offers the first large unbiased sample for the examination of correlations between different wavelength bands. We find that the near-IR nuclear J-and K-band luminosity is related to the BAT (14-195 keV) luminosity over a factor of 10(3) in luminosity (L-IR approximate to L-BAT(1.25)) and thus is unlikely to be due to dust. We also find that the Eddington ratio is proportional to the X-ray luminosity. This new result should be a strong constraint on models of the formation of the broadband continuum.
引用
收藏
页码:L65 / L68
页数:4
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