GRANAT/ART-P observations of GX3+1: Type I X-ray burst and persistent emission

被引：0
|
作者：
Molkov, SV [1 ]
Grebenev, SA
Pavlinsky, MN
Sunyaev, RA
机构：
[1] Russian Acad Sci, Inst Space Res, Moscow V71, Russia
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源：
ASTROPHYSICAL LETTERS & COMMUNICATIONS | 1999年 / 38卷 / 1-6期
关键词：
neutron star; accretion; boundary layer; X-ray burst; electron scattering;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present results of observations of the known LMXB source GX3+1 with the telescope ART-P on board GRANAT in the fall of 1990. A strong X-ray burst was detected from the source on Oct. 14 when it was in the low X-ray state with a luminosity similar to 30% smaller than the normal one. That was only the second case for the whole history of its study when it exhibited such type of activity. We describe results of the source spectroscopy during the bunt and persistent State and discuss formation of its X-ray emission in the accretion disk boundary Layer. It is noted that scattering on electrons plays the dominant role in the emission processes.
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收藏
页码：141 / 144
页数：4
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