Polarization of X-ray emission from the Sgr B2 cloud

被引:37
作者
Churazov, E
Sunyaev, R
Sazonov, S
机构
[1] Max Planck Inst Astrophys, D-85741 Garching, Germany
[2] Moscow Space Res Inst, Moscow 117810, Russia
关键词
polarization; scattering; ISM : individual : Sgr B2; Galaxy : centre; X-rays : general;
D O I
10.1046/j.1365-8711.2002.05113.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Sgr B2 giant molecular cloud is claimed to be an 'X-ray reflection nebula' - the reprocessing site of a powerful flare of the Sgr A* source, which occurred a few hundred years ago. The shape of the X-ray spectrum and the strength of the iron fluorescent line support this hypothesis. We argue that the cleanest test of the origin of X-rays from Sgr B2 would be a detection of polarized emission from this source.
引用
收藏
页码:817 / 820
页数:4
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