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Crust Cooling of Soft X-Ray Transients——the Uncertainties of Shallow Heating
引用本文:Xiang-Yang Lu,Guo-Liang Lü,He-Lei Liu,Chun-Hua Zhu,Zhao-Jun Wang.Crust Cooling of Soft X-Ray Transients——the Uncertainties of Shallow Heating[J].天文和天体物理学研究(英文版),2022(5):167-177.
作者姓名:Xiang-Yang Lu  Guo-Liang Lü  He-Lei Liu  Chun-Hua Zhu  Zhao-Jun Wang
作者单位:1. School of Physical Science and Technology, Xinjiang University;2. Center for Theoretical Physics, Xinjiang University
基金项目:supported by the Natural Science Foundation of Xinjiang Province under Grant No. 2020D01C063;;the National Natural Science Foundation of China (NSFC, Grant Nos. 11763007, U2031204 and 11863005);
摘    要:Crust cooling of soft X-ray transients has been observed after outbursts,but an additional shallow heating during accretion in outburst is needed to explain the quiescent light curve.However,shallow heating is significantly different between sources and even within one source between different outbursts,and the source of shallow heat is as yet unknown.Using the open source code "dStar" which solves the fully general relativistic heat diffusion equation for the crust,we investigate the effect of ...

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