For gamma-ray bursts (GRBs), there may exist ring-shaped jet when the jet axis does not coincide with the spin axis of its source. Using some refined jet dynamics, we study multi-wavelength afterglow light curves for such ring-shaped jets. There is an obvious break in the afterglow light curve due to the beaming effect. We also investigate the effects of many key parameters on the light curves and then use our model to fit light curves of some GRBs.
机构:
Department of Astronomy, Nanjing University, Nanjing 210093, China
Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, ChinaDepartment of Astronomy, Nanjing University, Nanjing 210093, China
Xu, M.
Huang, Y.F.
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Department of Astronomy, Nanjing University, Nanjing 210093, China
Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, ChinaDepartment of Astronomy, Nanjing University, Nanjing 210093, China
机构:
UNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCEUNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCE
ELMADANI, A
FAVIER, JC
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UNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCEUNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCE
FAVIER, JC
HEMERY, P
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UNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCEUNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCE
HEMERY, P
SIGWALT, P
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UNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCEUNIV PARIS 06,CHIM MACROMOLEC LAB,URA 24,4 PL JUSSIEU,F-75252 PARIS 05,FRANCE