The low-luminosity tail of the GRB distribution: The case of GRB 980425

Details The low-luminosity tail of the GRB distribution: The case of GRB 980425 The low-luminosity tail of the GRB distribution: The case of GRB 980425

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ncimc..28..283d&link_type=abstract

Il Nuovo Cimento C, vol. 28, Issue 3, p.283

Physics

Scientific paper

The association of GRB 980425 with the nearby supernova SN 1998bw at z = 0.0085 implies the existence of a population of GRBs with an isotropic-equivalent luminosity which is about 104 times smaller than in classical cosmic GRBs. We investigate two scenarios to explain the peculiar properties of GRB 980425: a normal (intrinsically bright) GRB seen off-axis or an intrinsically weak GRB seen on-axis.

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