Broad iron Kα line at z=1.146

被引:11
作者
Comastri, A
Brusa, M
Civano, F
机构
[1] Osservatorio Astron Bologna, INAF, I-40127 Bologna, Italy
[2] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
关键词
galaxies : active; galaxies : individual : CXOJ 123716.7+621733; X-rays : galaxies;
D O I
10.1111/j.1365-2966.2004.07929.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a strong iron Kalpha line in the hard X-ray selected source CXOJ 123716.7+621733 in the Chandra Deep Field-North survey at z = 1.146. The analysis is made possible by the very deep exposure of similar to2 Ms and the low background of the Advanced CCD Imaging Spectrometer (ACIS). The line profile seems to be inconsistent with a narrow feature. The best-fitting solution is achieved with a broad line. Most of the flux in the broad component originates at energies below 6.4 keV with a shape similar to that expected from emission in the inner-most regions of the accretion disc.
引用
收藏
页码:L9 / L13
页数:5
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