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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DOI: 10.1093/mnras/sty2337
Abstract: A thermal soft X-ray component is often detected in low-level accreting neutron stars (NSs), but is not detected in low-level accreting stellar-mass black holes (BHs). In this paper, we investigate the origin of such a… read more here.
Keywords: thermal soft; ray component; ray; low level ... See more keywords