activity
20092017
most citedModelling the light curves of PSR B1259-63/LS 2883-II.The effects of anisotropic pulsar wind and Doppler-boosting

70 citations · 249 across the 14 of their papers we have counts for

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9 papers · 1 filter

astro-ph.HE2015

Radio Afterglows and Host Galaxies of Gamma-Ray Bursts

Long-Biao Li, Zhi-Bin Zhang, Yong-Feng Huang +5

Considering the contribution of the emission from the host galaxies of gamma-ray bursts (GRBs) to the radio afterglows, we investigate the effect of host galaxies on observations s…

astro-ph.HE2014★ 14 cited

Detecting Radio Afterglows of Gamma-Ray Bursts with FAST

Zhi-Bin Zhang, Si-Wei Kong, Yong-Feng Huang +2

Using the generic hydrodynamic model of Gamma-Ray Burst (GRB) afterglows, we calculate the radio afterglow light curves of low luminosity, high luminosity, failed and standard GRBs…

astro-ph.HE2012★ 70 cited

Modelling the light curves of PSR B1259-63/LS 2883-II.The effects of anisotropic pulsar wind and Doppler-boosting

S. W. Kong, K. S. Cheng, Y. F . Huang

PSR B1259-63/LS 2883 is a binary system in which a 48-ms pulsar orbits around a Be star in a high eccentric orbit with a long orbital period of about 3.4 yr. It is special for havi…

astro-ph.HE2011★ 5 cited

The non-ballistic superluminal motion in the plane of the sky-II

Biping Gong, S. W. Kong, F. Xue +2

The model of non-ballistic jet motion proposed in 2008 provides a simple explanation to the inward jet motion and bent jet. Recently, evidences of such a non-radial motion increase…

astro-ph.HE2011★ 36 cited

Modeling the multi-wavelength light curves of PSR B1259-63/SS 2883

S. W. Kong, Y. W. Yu, Y. F. Huang +1

PSR B1259-63/SS 2883 is a binary system in which a 48-ms pulsar orbits around a Be star in a high eccentric orbit with a long orbital period of about 3.4 yr. Extensive broadband ob…

astro-ph.HE2010★ 4 cited

Measuring the beaming angle of GRB 030329 by fitting the rebrightenings in its multiband afterglow

Wei Deng, Yong-Feng Huang, Si-Wei Kong

Multiple rebrightenings have been observed in the multiband afterglow of GRB 030329. Especially, a marked and quick rebrightening occurred at about t ~ 1.2 * 10^5 s. Energy injecti…