The GRB980425-SN1998bw Association in the EMBH Model

Details The GRB980425-SN1998bw Association in the EMBH Model The GRB980425-SN1998bw Association in the EMBH Model

2004-07-07

arxiv.org/abs/astro-ph/0407147v1

AIP Conf.Proc. 727 (2004) 424-427

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure, to appear in the Proceedings of the Los Alamos "Gamma Ray Burst Symposium" in Santa Fe, New Mexico, Septemb

Scientific paper

10.1063/1.1810879

Our GRB theory, previously developed using GRB 991216 as a prototype, is here applied to GRB 980425. We fit the luminosity observed in the 40--700 keV, 2--26 keV and 2--10 keV bands by the BeppoSAX satellite. In addition the supernova SN1998bw is the outcome of an ``induced gravitational collapse'' triggered by GRB 980425, in agreement with the GRB-Supernova Time Sequence (GSTS) paradigm (\citet{lett3}). A further outcome of this astrophysically exceptional sequence of events is the formation of a young neutron star generated by the SN1998bw event (\citet{cospar02}). A coordinated observational activity is recommended to further enlighten the underlying scenario of this most unique astrophysical system.

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