activity
20072009
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 · 361 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE200943 cited

Observational Evidence for Young Radio Galaxies are Triggered by Accretion Disk Instability

Qingwen Wu

The bolometric luminosities and black hole (BH) masses are estimated by various methods for a sample of young radio galaxies with known ages. We find that the ages are positively c…

astro-ph.GA200956 cited

On the BL Lacertae objects/radio quasars and the FRI/II dichotomy

Ya-Di Xu, Xinwu Cao, Qingwen Wu

In the frame of unification schemes for radio-loud active galactic nuclei (AGNs), FR I radio galaxies are believed to be BL Lacertae (BL Lac) objects with the relativistic jet misa…

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-ph200843 cited

Jet power extracted from ADAF and the applications to X-ray binaries and radio galaxy FR dichotomy

Qingwen Wu, Xinwu Cao

We calculate the jet power of the classical Blandford-Znajek(BZ) model and hybrid model developed by Meier based on the global solutions of advection dominated accretion flows (ADA…

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…