XMM-Newton observations of the BL Lac MS 0737+7441

被引:1
作者
Boller, T
Gliozzi, M
Griffiths, G
Sembay, S
Keil, R
Schwentker, O
Brinkmann, W
Vercellone, S
机构
[1] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[2] Univ Leicester, Dept Phys & Astron, Xray Astron Grp, Leicester LE1 7RH, Leics, England
[3] CNR, Ist Fis Cosm G Occhialini, Milan, Italy
来源
ASTRONOMY & ASTROPHYSICS | 2001年 / 365卷 / 01期
关键词
galaxies : active; galaxies : individual : MS 0737.9+7441; X-rays : galaxies;
D O I
10.1051/0004-6361:20000055
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the XMM-Newton observations of the BL Lac object MS 0737.9 + 7841 during the performance verification phase. A simple power-law fit provides an adequate description of the integrated spectrum in the 0.2-10 keV energy band. The photon index is slightly steeper in the EPIC pn data with Gamma = (2.38 +/- 0.01) compared to the EPIC MOS data (Gamma = (2.28 +/- 0.01)). The difference is most probably due to the present uncertainties in the calibration of the EPIC MOS and EPIC pn data sets. We report evidence for intrinsic absorption in the distant BL Lac above the Galactic column (N-H,N-Gal = 32 1020 cm(-2)) which is N-H,fit(z=0.315) = (2.70 +/- 0.20) 10(20) cm(-2) in the EPIC pn data and N-H,fit(z=0.315) = (3.25 +/- 0.25) 10(20) cm(-2) in the EPIC MOS data assuming neutral gas and solar abundances. The flux variations are found to be of the order of 10%. No significant spectral variability is detected.
引用
收藏
页码:L158 / L161
页数:4
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