Can GRB early X-ray afterglows be explained by a contribution from the reverse shock?

Details Can GRB early X-ray afterglows be explained by a contribution from the reverse shock? Can GRB early X-ray afterglows be explained by a contribution from the reverse shock?

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..836..313g&link_type=abstract

GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference. AIP Conference Proceedings, Volume 836, pp. 313-

Astronomy and Astrophysics

Astrophysics

1

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

Scientific paper

We propose to explain the recent observations of early X-ray afterglows
by SWIFT from the dissipation of energy in the reverse shock sweeping
back into the ejecta. We compute the evolution of the dissipated power
and discuss the possibility that it can be radiated in the X-ray range.

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