Erlin Qiao

Identification of a new γ-ray-emitting narrow-line Seyfert 1 galaxy, at redshift ∼1

We report on the identification of a new

DISK CORONA INTERACTION: MECHANISM FOR THE DISK TRUNCATION AND SPECTRUM CHANGE IN LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI

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A disc corona–jet model for the radio/X-ray correlation in black hole X-ray binaries

-ray-emitting narrow-line Seyfert 1 (NLS1) galaxy, SDSS J122222.55+041315.7, which increases the number of known objects of this remarkable but rare type of active galactic nuclei (AGN) to seven. Its optical spectrum, obtained in the Sloan Digital Sky Survey-Baryon Oscillation Spectroscopic Survey, reveals a broad H

THE STRUCTURE AND SPECTRAL FEATURES OF A THIN DISK AND EVAPORATION-FED CORONA IN HIGH-LUMINOSITY ACTIVE GALACTIC NUCLEI

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A HYBRID TWO COMPONENT ACCRETION FLOW SURROUNDING SUPERMASSIVE BLACK HOLES IN AGNs

emission line with a width (FWHM) of 1734

The Disk Evaporation Model for the Spectral Features of Low-luminosity Active Galactic Nuclei

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Centrally Concentrated X-Ray Radiation from an Extended Accreting Corona in Active Galactic Nuclei

104 km s

REVISITING THE STRUCTURE AND SPECTRUM OF THE MAGNETIC-RECONNECTION-HEATED CORONA IN LUMINOUS AGNs

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Interaction of the accretion flows in corona and disk near the black hole in active galactic nuclei

. This, along with strong optical Fe II multiplets [

Do Long-cadence Data of the Kepler Spacecraft Capture Basic Properties of Flares?

R_{4570}=0.9