supported by the National Natural Science Foundation of China (Grants Nos.11025313, 10873002 and 11078008);National Basic Research Program of China (973 Program, Grant No.2009CB824800);Chinese Academy of Sciences (Grant KJCXZ-YW-T19);Guangxi SHI-BAI-QIAN project (Grant No.2007201);Guangxi Science Foundation (2010GXNSFC013011, 2011-135)
Swift GRB 100418A is a long burst at z = 0.624 without detection of any associated supernova (SN). Its light curves in both the prompt and afterglow phases are similar to GRB 060614, a nearby long GRB without an ass...
supported by the National Basic Research Program of China (Grant No. 2009CB824800);the National Natural Science Foundation of China (Grant No. 10873002); Guangxi SHI-BAI-QIAN Project (Grant No. 2007201);the Program for 100 Young and Middle-aged Disciplinary Leaders in Guangxi Higher Education Institutions,and the Research Foundation of Guangxi University (Grant No. M30520)
With the prompt slewing capability of the X-ray and UV-optical telescopes onboard the Swift mission and with the gamma-ray large area telescope onboard the Fermi mission,gamma-ray bursts(GRBs) are now accessible in a ...
supported by the National Natural Science Foundation of China (Grant Nos. 10821061, 10733010, 10725313, and 10873002);the National Basic Research Program of China (Grant No. 2009CB824800);Guangxi SHI-BAI-QIAN Project (Grant No. 2007201);the Program for 100 Young and Middle-aged Disciplinary Leaders in Guangxi Higher Education Institutions, the Research Foundation of Guangxi University (Grant No. M30520);the Ministry of Education of China, Directional Research Project of the Academy of Sciences (Grant No. KJCX2-YW-T03)
GRB 090423 is the new high-z record holder of Gamma-ray bursts(GRBs) with z-8.2.We present a detailed analysis of both the spectral and temporal features of GRB 090423 observed with Swift/BAT and Fermi/GBM.We find tha...
support by the National Basic Research Program of China (Grant No. 2009CB824800);the National Natural Science Foundation of China (Grant No. 10873002);Guangxi SHI-BAI-QIAN Project (Grant No. 2007201);the Program for 100 Young and Middle-aged Disciplinary Leaders in Guangxi Higher Education Instituions,and the Research Foundation of Guangxi University (Grant No. M30520)
With a sample of 58 Fermi/GBM GRBs detected before 2009 May,we compare the spectral properties of GBM GRBs with those detected by CGRO/BTASE and HETE-2.Our results show that the spectral index distributions are very c...
supported by the National Natural Science Foundation of China (Grant Nos.10747001, 10873002, and 10847003);the National Basic Research Program of China (Grant No. 2009CB824800), and the Research Foundation of Guangxi University (Grant No. M30520)
Using time-resolved spectral data for a sample of 30 pulses in 27 bright GRBs detected with CGRO/BATSE, we investigate the luminosity-peak energy relation (L-E p relation) in the decay phases of these pulses. A tight ...
Supported by the National Natural Science Foundation of China (Grant Nos. 10573002, 10778611, and 10873002); the National Basic Research Program of China (Grant No. 2009CB824800);the Research Foundation of Guangxi University (Grant No. M30520);the LCWR (Grant No. LHXZ200602)
A star-quake model is proposed to understand X-ray flares of both long and short γ-ray bursts (GRBs) in a solid quark star regime. Two kinds of central engines for GRBs are available if pulsar-like stars are actually...