XMM-Newton observations of absorption features towards PKS 2155-304

被引:3
作者
Cagnoni, I
Nicastro, F
Maraschi, L
Treves, A
Tavecchio, F
机构
[1] Univ Insubria, Dip Sci, I-22100 Como, Italy
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[3] Osserv Astron Brera, I-20121 Milan, Italy
关键词
BL lacertae objects; individual (PKS 2155-304); intergalactic medium; large-scale structure of universe; quasars; absorption lines;
D O I
10.1016/S1387-6473(03)00093-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present XMM-Newton grating spectra of the bright BL Lac object PKS 2155 - 304 taken in November 2000. Various absorption features are detected in the range 5-38 A. The results are compared with those recently obtained with Chandra gratings [ApJ 573 (2002) 157; Nature, 421 (2003) 719]. We discuss whether the absorption occurs at the source (in the host galaxy or in a jet), in the Galactic halo, or in the intervening cluster. We are not able to confirm the proposal by [ApJL 572 (2002) L127] that a hot medium is responsible for an absorption feature at an intermediate redshift. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:561 / 563
页数:3
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