activity
20042023
most citedStar formation in self-gravitating disks in active galactic nuclei. I. Metallicity gradients in broad line regions

51 citations · 114 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2023★ 5 cited

The year-scale X-ray variations in the core of M87

Yu-Lin Cheng, Fei Xiang, Heng Yu +5

The analysis of light variation of M87 can help us understand the disc evolution. In the past decade, M87 has experienced several short-term light variabilities related to flares.…

astro-ph.HE2020★ 1 cited

Disk evolution of the M87's nucleus observed in 2008

Fei Xiang, Cheng Cheng

We report the discovery of year-scale X-ray variation in the nuclear region of the M87 by reanalyzing the 8 Chandra observations from 2007 to 2008. The X-ray spectra are fitted and…

astro-ph.CO2012★ 5 cited

Deprojected analysis of Abell 1835 observed with Chandra and compared with XMM-Newton

Chengkui Li, Shumei Jia, Yong Chen +3

Using a deprojection technique, we study the X-ray properties of the galaxy cluster Abell 1835 observed with Chandra, including temperature, abundance, electron density, gas mass f…

astro-ph.GA2011★ 51 cited

Star formation in self-gravitating disks in active galactic nuclei. I. Metallicity gradients in broad line regions

J. -M. Wang, J. -Q. Ge, C. Hu +6

It has been suggested that the high metallicity generally observed in active galactic nuclei (AGNs) and quasars originates from ongoing star formation in the self-gravitating part…

astro-ph.CO2009★ 15 cited

Evolution of gaseous disk viscosity driven by supernova explosion in star-forming galaxies at high redshift

Jian-Min Wang, Chang-Shuo Yan, Yan-Rong Li +5

Motivated by Genzel et al.'s observations of high-redshift star-forming galaxies, containing clumpy and turbulent rings or disks, we build a set of equations describing the dynamic…

astro-ph2007★ 23 cited

On the width of cold fronts in clusters of galaxies due to conduction

F. Xiang, E. Churazov, K. Dolag +2

We consider the impact of thermal conduction in clusters of galaxies on the (unmagnetized) interface between a cold gaseous cloud and a hotter gas flowing over the cloud (the so-ca…