Gamma-ray bursts from internal shocks in a relativistic wind: Temporal and spectral properties

Details Gamma-ray bursts from internal shocks in a relativistic wind: Temporal and spectral properties Gamma-ray bursts from internal shocks in a relativistic wind: Temporal and spectral properties

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..772m&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 772-776 (1996).

Computer Science

1

Gamma-Ray Sources, Gamma-Ray Bursts, Radiation Mechanisms, Polarization, Mass Loss And Stellar Winds

Scientific paper

We present a simple model to test the proposal by Rees and
Mészáros (1994) that GRBs could result from internal
shocks in a relativistic wind. We compute both time profiles and spectra
for synthetic bursts. Some of the properties of real bursts, such as the
duration-hardness ratio relation, are recovered.

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