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

136 citations

Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2011136 cited

Kinematics and Fine Structure of An Unwinding Polar Jet Observed by SDO/AIA

Yuandeng Shen, Yu Liu, Jiangtao Su +1

We present an observational study of the kinematics and fine structure of an unwinding polar jet, with high temporal and spatial observations taken by the Atmospheric Imaging Assem…

astro-ph.SR201127 cited

Period changes and four-color light curves of the active overcontact binary v396 monocerotis

Liu Liang, Qian Shengbang, Liao Wenping +4

This paper analyzes the first secured four color light curves of V396 Mon using the 2003 version of the WD code. It is confirmed that V396 Mon is a shallow W-type contact binary sy…

astro-ph.SR201113 cited

SS Ari: a shallow-contact close binary system

Liu Liang, Qian Shengbang, He Jiajia +2

Two CCD epochs of light minimum and a complete R light curve of SS Ari are presented. The light curve obtained in 2007 was analyzed with the 2003 version of the W-D code. It is sho…

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.SR200957 cited

Detection of a tertiary brown dwarf companion in the sdB-type eclipsing binary HS 0705+6700

S. Qian, L. Zhu, S. Zola +6

HS 0705+6700 is a short-period (P=2.3 hours), close binary containing a hot sdB-type primary and a fully convective secondary. We have monitored this eclipsing binary for more than…