On GRB 080916C and GRB 090902B observed by the Fermi satellite

Details On GRB 080916C and GRB 090902B observed by the Fermi satellite On GRB 080916C and GRB 090902B observed by the Fermi satellite

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1279..343i&link_type=abstract

DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS. AIP Conference Proceedings, Volume 1279, pp. 343-345 (2010).

Astronomy and Astrophysics

Astronomy

Gamma-Ray Sources (Astronomical), Interstellar Matter, Interstellar Molecular Clouds, Gamma-Ray Sources, Gamma-Ray Bursts, Physical Properties, Molecular Clouds, H2 Clouds, Dense Clouds, And Dark Clouds

Scientific paper

We propose a possible explanation, in the context of the Fireshell scenario, for the high-energy emission observed in GRB 080916C and GRB 090902B. The physical process underlying this emission consists mainly in the interaction of the baryon in the Fireshell with some high-density region around the burst site. Moreover we associate the observed delay of the onset of the high-energy emission as due to the P-GRB emission.

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