WAS AN OUTBURST OF AQUILA X-1 A MAGNETIC FLARE?

被引:4
|
作者
Soker, Noam [1 ]
机构
[1] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel
基金
以色列科学基金会;
关键词
stars: flare; X-rays: binaries; X-RAY; DWARF NOVA; SOLAR-FLARES; LIGHT CURVES; SS-CYGNI; EVOLUTION; CORONAE; EVAPORATION; EJECTIONS; EMISSION;
D O I
10.1088/2041-8205/721/2/L189
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I point to an interesting similarity in the radio and the soft X-ray light curves between the 2009 November outburst of the X-ray binary Aquila X-1 and some solar flares. The ratio of the soft X-ray and radio luminosities of Aquila X-1 in that outburst is also similar to some weak solar flares, as is the radio spectrum near 8 GHz. Based on these as well as on some other recent studies that point to some similar properties of accretion disk coronae and stellar flares, such as the ratio of radio to X-ray luminosities, I speculate that the soft X-ray outburst of Aquila X-1 was related to a huge magnetic flare from its disk corona.
引用
收藏
页码:L189 / L192
页数:4
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