ROSAT PSPC detection of soft X-ray absorption in GB 1428+4217:: the most distant matter yet probed with X-ray spectroscopy

被引:14
作者
Boller, T
Fabian, AC
Brandt, WN
Freyberg, MJ
机构
[1] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[2] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[3] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
关键词
galaxies : active; galaxies : individual : GB 1428+4217; X-rays : galaxies;
D O I
10.1046/j.1365-8711.2000.03635.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on a ROSAT PSPC observation of the highly luminous z = 4.72 radio-loud quasar GB 1428+4217 obtained between 1998 December 11 and 17, the final days of the ROSAT satellite. The low-energy sensitivity of the PSPC detector was employed to constrain the intrinsic X-ray absorption of the currently most distant X-ray detected object. Here we present the detection of significant soft X-ray absorption towards GB 1428+4217, making the absorbing material the most distant matter yet probed with X-ray spectroscopy. X-ray variability by 25 +/- 8 per cent is detected on a time-scale of 6500 s in the rest frame. The X-ray variation requires an unusually high radiative efficiency eta of at least 4.2, further supporting the blazar nature of the source.
引用
收藏
页码:L23 / L28
页数:6
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