activity
20042009
most citedThe hard X-ray spectral evolution in X-ray binaries and its application to constrain the black hole mass of ultraluminous X-ray sources

142 citations · 339 across the 6 of their papers we have counts for

collaborators
Showing astro-phShow all

5 papers · 1 filter

astro-ph2008

The Hard X-ray Spectral Evolution in XRBs, AGNs and ULXs

Qingwen Wu, Minfeng Gu

We explore the relationship between the hard X-ray photon index and the Eddington ratio (ξ=L_{X}(0.5-25 keV)/L_{Edd}) in six XRBs. We find that different XRBs follow different…

astro-ph2008142 cited

The hard X-ray spectral evolution in X-ray binaries and its application to constrain the black hole mass of ultraluminous X-ray sources

Qingwen Wu, Minfeng Gu

We investigate the relationship between the hard X-ray photon index and the Eddington ratio () in six X-ray binaries (XRBs) with well constrain…

astro-ph200777 cited

On the origin of X-ray emission in some FR Is: ADAF or jet?

Qingwen Wu, Feng Yuan, Xinwu Cao

We investigate the X-ray origin in FR Is using the radio, submillimetre, optical, and {\em Chandra} X-ray data of a small sample consisting of eight FR I sources. These sources are…

astro-ph200621 cited

The relation between star formation rate and accretion rate in LINERs

Qingwen Wu, Xinwu Cao

It is argued that there is a linear correlation between star formation rate (SFR) and accretion rate for normal bright active galactic nuclei (AGNs). However, it is still unclear w…

astro-ph2004

Origin of Radio Emission from Nearby Low-Luminosity Active Galactic Nuclei

Qingwen Wu, Xinwu Cao

We use the observational data in radio, optical and X-ray wavebands, for a sample of active galactic nuclei (AGNs) with measured black hole masses, to explore the origin of radio e…