output
20022013
most citedResults of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006-2007

136 citations

Showing 2009Show all

7 papers · 1 filter

astro-ph.CO200912 cited

Metal-Enriched Outflows in the Ultra-Luminous infrared Quasar Q1321+058

Tinggui Wang, Hongyan Zhou, Weimin Yuan +3

Quasar outflows may play important role in the evolution of its host galaxy and central black hole. In this paper, we present a detailed study of multiple outflows in the obscured…

astro-ph.GA200962 cited

Eddington ratio governs the equivalent width of MgII emission line in active galactic nuclei

Xiao-Bo Dong, Ting-Gui Wang, Jian-Guo Wang +4

We have investigated the ensemble regularities of the equivalent widths (EWs) of MgII 2800 emission line of active galactic nuclei (AGNs), using a uniformly selected sample of 2092…

astro-ph.SR200924 cited

Nonaxisymmetric Rossby Vortex Instability with Toroidal Magnetic Fields in Radially Structured Disks

Cong Yu, Hui Li

We investigate the global nonaxisymmetric Rossby vortex instability in a differentially rotating, compressible magnetized accretion disk with radial density structures. Equilibrium…

astro-ph.SR2009106 cited

Numerical Experiments of Wave-Like Phenomena Caused by the Disruption of an Unstable Magnetic Configuration

Hongjuan Wang, Chengcai Shen, Jun Lin

The origin of the Moreton wave observed in the chromosphere and the EIT wave observed in the corona during the eruption remains being an active research subject for a while. We inv…

astro-ph.GA20094 cited

The origin and physical mechanism of the ensemble Baldwin effect

Xiaobo Dong, Jianguo Wang, Tinggui Wang +5

We have conducted a systematic investigation of the origin and underlying physics of the line--line and line--continuum correlations of AGNs, particularly the Baldwin effect. Based…

astro-ph.HE200961 cited

Rise and fall of the X-ray flash 080330: an off-axis jet?

C. Guidorzi, C. Clemens, S. Kobayashi +31

X-ray flashes (XRFs) are a class of gamma-ray bursts (GRBs) with the peak energy of the time-integrated spectrum, Ep, below 30 keV, whereas classical GRBs have Ep of a few hundreds…