Long-term flaring activity of XRF 011030 observed with BeppoSAX

被引:22
|
作者
Galli, A. [1 ]
Piro, L. [1 ]
机构
[1] INAF, Ist Astrofis Spaziale & Fis Cosm, Sez Roma, I-00133 Rome, Italy
关键词
radiation mechanism : non-thermal; gamma rays : bursts;
D O I
10.1051/0004-6361:20054448
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the spectral and temporal analysis of the X-ray flash XRF 011030 observed with BeppoSAX. This event is characterized by a very long X-ray bursting activity that lasts about 1500 s, one of the longest ever observed by BeppoSAX. In particular, a precursor and a late flare are present in the light curve. We connect the late X-ray flare observed at about 1300 s to the afterglow emission observed by Chandra and associate it with the onset of the afterglow emission in the framework of external shock by a long duration engine activity. We find that the late X-ray flare and the broadband afterglow data, including optical and radio measurements, are consistent either with a fireball expanding in a wind environment or with a jetted fireball in an ISM.
引用
收藏
页码:413 / 422
页数:10
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