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.


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    Titel :

    GRB 980425, SN1998BW and the EMBH model


    Beteiligte:
    Ruffini, R. (Autor:in) / Bernardini, M.G. (Autor:in) / Bianco, C.L. (Autor:in) / Chardonnet, P. (Autor:in) / Fraschetti, F. (Autor:in) / Xue, S.-S. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 34 , 12 ; 2715-2722


    Erscheinungsdatum :

    2003-06-10


    Format / Umfang :

    8 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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