The advection-dominated accretion flow for the origin of the thermal soft X-ray component in low-level accreting neutron stars

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2018-11, Vol.481 (1), p.938-946
Main Authors: Qiao, Erlin, Liu, B F
Format: Article
Language:English
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ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/sty2337