Origin of XRFs: low Ė, low contrast of Γ or large viewing angle?

Details Origin of XRFs: low Ė, low contrast of Γ or large viewing angle? Origin of XRFs: low Ė, low contrast of Γ or large viewing angle?

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..101b&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 101-105 (2004).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray Sources, X-Ray Bursts

Scientific paper

We have developed a toy model for internal shocks which has been used to
produce a large number of synthetic GRB/XRF events in order to find the
critical parameters for the production of X-ray flashes. The key factor
appears to be a small contrast of the Lorentz factor in the relativistic
outflow emitted by the central engine.

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