Effects of the Core-collapse Supernova Ejecta Impact on a Rapidly Rotating Massive Companion Star
Effects of the Core-collapse Supernova Ejecta Impact on a Rapidly Rotating Massive Companion Star
复制标题
核心塌缩超新星抛射物撞击快速旋转的大质量伴星的影响
DOI：
10.3847/1538-4357/aa56c2
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发表时间：
2017-01
影响因子：
4.9
通讯作者：
Wang Zhaojun
中科院分区：
文献类型：
--
作者：
Zhu Chunhua;Lu Guoliang;Wang Zhaojun
我们研究了核心 - 循环超新星（CCSN）弹出对快速旋转和巨大的伴侣恒星的影响。我们表明，被剥离的质量是庞大但不旋转的伴侣明星的两倍。用轨道p的近距离二进制
We investigate the effects of the core-collapse supernova (CCSN) ejecta on a rapidly rotating and massive companion star. We show that the stripped mass is twice as high as that of a massive but nonrotating companion star. In close binaries with orbital periods of about 1 day, the stripped masses reach up to . By simulating the evolutions of the rotational velocities of the massive companion stars based on different stripped masses, we find that the rotational velocity decreases greatly for a stripped mass higher than about . Of all the known high-mass X-ray binaries (HMXBs), Cygnus X-3 and 1WGA J0648.024418 have the shortest orbital periods, 0.2 and 1.55 days, respectively. The optical counterpart of the former is a Wolf-Rayet star, whereas it is a hot subdwarf for the latter. Applying our model to the two HMXBs, we suggest that the hydrogen-rich envelopes of their optical counterparts may have been stripped by CCSN ejecta.
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DOI：
10.1046/j.1365-8711.2002.05752.x
发表时间：
2002-06
影响因子：
4.8
作者：
Zhanwen Han;P. Podsiadlowski;P. Maxted;T. Marsh;N. Ivanova
通讯作者：
Zhanwen Han;P. Podsiadlowski;P. Maxted;T. Marsh;N. Ivanova
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DOI：
10.1046/j.1365-8711.2002.05038.x
发表时间：
2002-01
影响因子：
4.8
作者：
J. Hurley;C. Tout;O. Pols
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DOI：
10.1007/s00159-013-0069-0
发表时间：
2003-10
影响因子：
3.5
作者：
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J. Porter;T. Rivinius
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