activity
20072009
most citedAn accretion disc-corona model for X-ray spectra of active galactic nuclei

103 citations · 297 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20094 cited

SDSS spectroscopy for blazars in the LAT bright AGN sample

Zhaoyu Chen, Minfeng Gu, Zhonghui Fan +1

We have collected all available spectra and photometric data from SDSS catalogue for bright AGNs complied from the first three months of the Fermi large area telescope all-sky surv…

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-ph2008103 cited

An accretion disc-corona model for X-ray spectra of active galactic nuclei

Xinwu Cao

The hard X-ray emission of active galactic nuclei (AGN) is believed to originate from the hot coronae above the cold accretion discs. The hard X-ray spectral index is found to be c…

astro-ph200814 cited

The advection-dominated accretion flow+thin accretion disk model for two low-luminosity active galactic nuclei: M81 and NGC4579

Ya-Di Xu, Xinwu Cao

It was found that the advection-dominated accretion flow (ADAF)+thin disk model calculations can reproduce the observed spectral energy distributions (SED) of the two low luminosit…

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-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…