GRB970228 as a Prototype for the Class of GRBs with AN Initial Spikelike Emission

Physics

Scientific paper

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Gamma Rays: Bursts, Black Hole Physics, Galaxies: Halos

Scientific paper

We interpret GRB970228 prompt emission within our "canonical" GRB
scenario, identifying the initial spikelike emission with the Proper-GRB
(P-GRB) and the following bumps with the afterglow peak emission.
Furthermore, we emphasize the necessity to consider the "canonical" GRB
as a whole due to the highly non-linear nature of the model we applied.

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