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

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..328d&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 328-332 (2004).

Mathematics

Logic

1

Gamma-Ray Sources, Gamma-Ray Bursts, Supernovae

Scientific paper

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

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