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2.Qiao, Erlin, Liu, B.F.,“The advection-dominated accretion flow for the anticorrelation between the X-ray photon index and the X-ray luminosity in neutron star low-mass X-ray binaries”, 2020b, MNRAS, 496, 2704
3.Qiao, Erlin, Liu, B.F.,“A systematic study of the advection-dominated accretion flow for the origin of the X-ray emission in weakly magnetized low-level accreting neutron stars”, 2020a, MNRAS, 492, 615
4.Qiao, Erlin, Liu, B.F.,“A model for the radio/X-ray correlation in three neutron star low-mass X-ray binaries 4U 1728-34, Aql X-1, and EXO 1745-248”, 2019, MNRAS, 487, 1626
5.Qiao, Erlin, Liu, B.F.,“The advection-dominated accretion flow for the origin of the thermal soft X-ray component in low-level accreting neutron stars”, 2018b, MNRAS, 481, 938
具体可查看我的ADS链接:https://ui.adsabs.harvard.edu/public-libraries/F65cYq8wTgeNdwp8LSmnug