On the Possible Nature of Be/X X-Ray Luminosity

被引：0
|
作者：
Kaygorodov, P. V. [1 ]
Bisikalo, D. V. [1 ]
Kononov, D. A. [1 ]
Boneva, D. V. [2 ]
机构：
[1] Russian Acad Sci, Inst Astron, RU-119017 Moscow, Russia
[2] Bulgarian Acad Sci, Sp Res & Technol Inst, B-1113 Sofia, Bulgaria
来源：
SPACE PLASMA PHYSICS | 2013年 / 1551卷
基金：
俄罗斯基础研究基金会;
关键词：
Be-stars; Be/X; X-ray; binary stars; accretion; MAGELLANIC-CLOUD; BINARY; STARS; DISCOVERY; PULSAR; ROSAT;
D O I：
10.1063/1.4818852
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A new mechanism for the generation of X-ray luminosity in binary Be/X-stars is proposed. Using the model of the expanding envelope of optical component of binary Be/X-star it was shown that the rate of mass transfer through the vicinity of L-1 is sufficient to generate the observed X-ray luminosity of Be/X-stars. The relationship between the orbital period of the system and the magnitude of X-ray flux was discovered. The relationship between the orbital period of the system and the mass transfer rate, obtained from the simulation results, corresponds to the observed dependence of the maximum X-ray flux during the outburst on the orbital period for binary Be/X stars.
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页数：7
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