XMM-Newton observations of Markarian 421

被引:38
作者
Brinkmann, W
Sembay, S
Griffiths, RG
Branduardi-Raymont, G
Gliozzi, M
Boller, T
Tiengo, A
Molendi, S
Zane, S
机构
[1] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[2] Univ Leicester, Dept Phys & Astron, Xray Astron Grp, Leicester LE1 7RH, Leics, England
[3] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[4] XMM Newton Sci Operat Ctr, Villafranca Satellite Tracking Stn, Madrid 28080, Spain
[5] Ist Fis Cosm G Occhialini, I-20133 Milan, Italy
来源
ASTRONOMY & ASTROPHYSICS | 2001年 / 365卷 / 01期
关键词
BL Lac objects - general; galaxies : active - quasars; X-rays : general; radio sources : general;
D O I
10.1051/0004-6361:20000084
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The BL Lac object Mrk 421 was observed on May 25, 2000 during the XMM-Newton Cal/PV phase. The high throughput of the X-ray telescopes and the spectral capabilities of the instruments allow an uninterrupted temporal and spectral study of the source with unprecedented time resolution. Mrk 421 was found at a relatively high state with a 2-6 keV flux of (1.3-1.9) 10(-10) erg cm(-2) s(-1). The observed intensity variations by more than a factor of three at highest X-ray energies are accompanied by complex spectral variations with only a small time lag (tau = 265(-102)(+116) s) between the hard and soft photons. The (0.2-10) keV spectrum can be well fitted by a broken power law and no absorption structures are found in the source spectrum at the high spectral resolution of the transmission gratings.
引用
收藏
页码:L162 / L167
页数:6
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