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Luminosity Limit of Super-Eddington Accretion onto Black Holes

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摘要 The luminosity limit is derived for the super-Eddington accretion by obtaining the self-similar solution.The maximum luminosity is about 4.0×10^(37) erg/s(M/M_(⊙))or so(significantly less than the Eddington luminosity)due to photon trapping although the accretion rate is super-Eddington.The radiation spectrum is found to be universal as F_(v) α v^(-1).
作者 WANG Jian-min 王建民(Department of Astronomy,Beijing Normal University,Beijing 100875;Chinese Academy of Sciences-Peking University Joint Beijing Astrophysical Center,Beijing 100871)
出处 《Chinese Physics Letters》 SCIE CAS CSCD 1999年第6期467-468,共2页 中国物理快报(英文版)
基金 Supported by Climbing Plan of the Ministry of Science and Technology of China,and the National Natural Science Foundation of China under Grant No.19803002.
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