Accretion;
accretion disk;
black hole physics;
shock Waves;
outflows;
D O I:
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摘要:
We self-consistently obtain shock locations in an accretion flow by using an analytical method. One can obtain the spectral properties, quasi-periodic oscillation frequencies and the outflow rates when the inflow parameters are known. Since temperature of the CENBOL decides the spectral states of the black hole, and also the outflow rate, the outflow rate is directly related to the spectral states.
机构:
Yunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R ChinaYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
Singh, Chandra B.
Okuda, Toru
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机构:
Hokkaido Univ, Hakodate Campus,Hachiman Cho 1-2, Hakodate, Hokkaido 0408567, JapanYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China
Okuda, Toru
Aktar, Ramiz
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机构:
Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R ChinaYunnan Univ, South Western Inst Astron Res, Kunming 650500, Yunnan, Peoples R China