Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-01-09
Astrophys.J. 607 (2004) L103-L106
Astronomy and Astrophysics
Astrophysics
13 pages, 4 eps figures
Scientific paper
10.1086/421872
Taking into account the recent suggestion that a short gamma-ray burst (GRB) looks like the first 1 sec of a long GRB, we propose that the jet of a GRB consists of multiple sub-jets or sub-shells (i.e., an inhomogeneous jet model). The multiplicity of the sub-jets along a line of sight n_s is an important parameter. If n_s is large (>> 1) the event looks like a long GRB, while if n_s is small (~1) the event looks like a short GRB. If our line of sight is off-axis to any sub-jets, the event looks like an X-ray flash or an X-ray rich GRB. The log-normal distribution of durations of short and long GRBs are also suggested in the same model.
Ioka Kunihito
Nakamura Takashi
Yamazaki Ryo
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