The 0.1-100 keV spectrum and variability of Mrk 421 in a high state

被引:26
作者
Malizia, A
Capalbi, M
Fiore, F
Giommi, P
Gandolfi, G
Tesseri, A
Antonelli, LA
Butler, RC
Celidonio, G
Coletta, A
Di Ciolo, L
Muller, JM
Piro, L
Rebecchi, S
Ricci, D
Ricci, R
Smith, M
Torroni, V
机构
[1] BeppoSAX Sci Data Ctr, I-00131 Rome, Italy
[2] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
[3] Telespazio SpA, I-00131 Rome, Italy
[4] Osserv Astron Roma, I-00044 Frascati, Italy
[5] BeppoSAX SOC, I-00131 Rome, Italy
[6] SRON, NL-3584 CA Utrecht, Netherlands
[7] CNR, Ist Astrofis Spaziale, I-00133 Rome, Italy
[8] ASI, Area Ric Sci, Rome, Italy
关键词
galaxies : active; BL Lacertae objects : individual : Mrk 421; X-rays : galaxies;
D O I
10.1046/j.1365-8711.2000.03106.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The results of a BeppoSAX target of opportunity (TOO) observation of the BL Lac object Mrk 421 during a high-intensity state are reported and compared with monitoring X-ray data collected with the BeppoSAX Wide Field Cameras (WFC) and the RXTE All Sky Monitor (ASM). The 0.1-100 keV spectrum of Mrk 421 shows continuous convex curvature that can be interpreted as the high-energy end of the synchrotron emission. The source shows significant short-term temporal and spectral variability, which can be interpreted in terms of synchrotron cooling. The comparison of our results with those of previous observations when the source was a factor 3-5 fainter shows evidence for strong spectral variability, with the maximum of the synchrotron power shifting to higher energy during high states. This behaviour suggests an increase in the number of energetic electrons during high states.
引用
收藏
页码:123 / 129
页数:7
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