AbstractThe EMBH model, 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 we present a novel scenario in which 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 [Ruffini, R., Bianco, C.L., Chardonnet, P., Fraschetti, F., Xue, S.-S. On a possible GRB-supernova time sequence. Astrophys. J. 555, L117–L120, 2001c]. A further outcome of this astrophysically exceptional sequence of events is the formation of a young neutron star generated by the SN1998bw event. A coordinated observational activity is recommended to further enlighten the underlying scenario of this most unique astrophysical system.
GRB 980425, SN1998BW and the EMBH model
Advances in Space Research ; 34 , 12 ; 2715-2722
2003-06-10
8 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
GRB 980425, SN1998BW and the EMBH Model
British Library Conference Proceedings | 2004
|GRB 980425, SN1998BW and the EMBH model
Online Contents | 2004
|XMM-Newton observations of the field of #947-ray burst 980425
Online Contents | 2004
|XMM-Newton Observations of the Field of gamma-Ray Burst 980425
British Library Conference Proceedings | 2004
|XMM-Newton observations of the field of γ-ray burst 980425
Elsevier | 2003
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