2015/11-present, Research professor at UCAS (part-time)

2013/09-present, Associate research professor at NAOC 

2012/11-2013/11, Assistant research professor at NAOC 

2010/11-2012/11, Postdoc at NAOC

2008/01-2009/01, Joint Ph.D student, Max Planck Institute for Astrophysics, Garching, Germany

2005/09-2010/07, Ph.D, University of Chinese Academy of Sciences (UCAS), China

High energy astrophysics 

Accretion theory for compact objects 

X-ray binaries 

Active galactic nuclei 

Tidal disruption events

1. We have established the “disk evaporation” and “corona condensation” model for black holes (BHs) from stellar-mass BH in X-ray binaries and super-massive BH in the center of galaxies

2. We have developed the “hot accretion flow” theory around the stellar-mass compact objects [neutron star (NS) and BH] for distinguishing the effect of the hard surface in NSs and the event horizon in BHs.

1. Qiao, Erlin, Liu, B. F. 2020. The advection-dominated accretion flow for the anticorrelation be- tween the X-ray photon index and the X-ray luminosity in neutron star low-mass X-ray binaries. Monthly Notices of the Royal Astronomical Society 496, 2704–2714.

2. Qiao, Erlin, Liu, B. F. 2020. 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. Monthly Notices of the Royal Astronomical Society 492, 615.

3. Qiao, Erlin, Liu, B. F. 2019. A model for the radio/X-ray correlation in three neutron star low-mass X-ray binaries 4U 1728-34, Aql X-1ad, and EXO 1745-248. Monthly Notices of the Royal Astronomical Society 487, 1626.

4. Qiao, Erlin, Liu, B. F. 2018. The advection-dominated accretion flow for the origin of the thermal soft X-ray component in low-level accreting neutron stars. Monthly Notices of the Royal Astronomical Society 481, 938.

5. Qiao, Erlin, Liu, B. F. 2018. A systematic study of the condensation of the corona and the ap- plication for Γ 2？10keV-Lbol/LEdd correlation in luminous active galactic nuclei. Monthly Notices of the Royal Astronomical Society 477, 210.

6.Qiao, Erlin, Liu, B. F. 2017. The condensation of the corona for the correlation between the hard X-ray photon index Γ and the reflection scaling factor R in active galactic nuclei. Monthly Notices of the Royal Astronomical Society 467, 898.

7. Qiao, Erlin, Liu, B. F. 2015. A disc corona-jet model for the radio/X-ray correlation in black hole X-ray binaries. Monthly Notices of the Royal Astronomical Society 448, 1099.

8. Qiao, Erlin, Liu, B. F., Panessa, F., Liu, J. Y. 2013. The Disk Evaporation Model for the Spectral Features of Low-luminosity Active Galactic Nuclei. The Astrophysical Journal 777, 102.

9. Qiao, Erlin, Liu, B. F. 2013. A Model for the Correlation of Hard X-Ray Index with Eddington Ratio in Black Hole X-Ray Binaries. The Astrophysical Journal 764, 2.

10.Qiao, Erlin, Liu, B. F. 2012. The Emission from an Inner Disk and a Corona in the Low and Intermediate Spectral States of Black Hole X-Ray Binaries. The Astrophysical Journal 744, 145.

See my full publication list (ADS):

https://ui.adsabs.harvard.edu/public-libraries/F65cYq8wTgeNdwp8LSmnug