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Zhang F.
Zhang B.
Zhang C. M.
Zhang Bing
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bzhang@physics.unlv.edu
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http://hub.abes.fr/oup/periodical/mnras/2007/volume_374/issue_3/101111j13652966200611226x/authorship/1
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http://hub.abes.fr/oup/periodical/mnras/2006/volume_366/issue_4/101111j13652966200609920x/authorship/1
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GRB 050223: a faint gamma-ray burst discovered by Swift
Diagnosing the site of gamma-ray burst prompt emission with spectral cut-off energy
Multiwavelength observations of the energetic GRB 080810: detailed mapping of the broad-band spectral evolution
The bottom magnetic field and magnetosphere evolution of neutron star in low-mass X-ray binary
The unusual X-ray emission of the short Swift GRB 090515: evidence for the formation of a magnetar?
Measuring neutron star mass and radius with three mass-radius relations
The Swift gamma-ray burst GRB 050422
Calibration of gamma-ray burst luminosity indicators
Prompt optical emission and synchrotron self-absorption constraints on emission site of GRBs
The late time evolution of gamma-ray bursts: ending hyperaccretion and producing flares
The unusual X-ray light curve of GRB 080307: the onset of the afterglow?
Swift and optical observations of GRB 050401
Can X-ray emission powered by a spinning-down magnetar explain some gamma-ray burst light-curve features?
High-energy afterglow emission from giant flares of soft gamma-ray repeaters: the case of the 2004 December 27 event from SGR 1806-20
Prompt emission of high-energy photons from gamma ray bursts
Extreme properties of GRB 061007: a highly energetic or a highly collimated burst?
γ-ray burst internal shocks with magnetization
Possible effects of pair echoes on gamma-ray burst afterglow emission
On the origins of part-time radio pulsars
Early afterglow detection in the Swift observations of GRB 050801
GRB 050505: a high-redshift burst discovered by Swift
The correlations between the twin kHz quasi-periodic oscillation frequencies of low-mass X-ray binaries
Is there evidence for field restructuring or decay in accreting magnetic white dwarfs?
Low-luminosity gamma-ray bursts as a distinct GRB population: a firmer case from multiple criteria constraints
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