GRB 980425, SN1998bw and the EMBH model

Details GRB 980425, SN1998bw and the EMBH model GRB 980425, SN1998bw and the EMBH model

2003-06-12

arxiv.org/abs/astro-ph/0306246v2

Adv.Sp.Res. 34 (2004) 2715-2722

Astronomy and Astrophysics

Astrophysics

10 pages, 3 figures, in the Proceedings of the 34th COSPAR scientific assembly, Elsevier. Fixed some typos in this new version

Scientific paper

10.1016/j.asr.2003.06.044

The 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 et al. 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.

Affiliated with

Also associated with

No associations

Rating

GRB 980425, SN1998bw and the EMBH model does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with GRB 980425, SN1998bw and the EMBH model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GRB 980425, SN1998bw and the EMBH model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-408573