Exact versus approximate equitemporal surfaces in Gamma-Ray Burst afterglows

Details Exact versus approximate equitemporal surfaces in Gamma-Ray Burst afterglows Exact versus approximate equitemporal surfaces in Gamma-Ray Burst afterglows

2004-03-16

arxiv.org/abs/astro-ph/0403379v1

Astrophys.J. 605 (2004) L1-L4

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, to appear on ApJ Lett

Scientific paper

10.1086/386367

By integrating the relativistic hydrodynamic equations introduced by Taub we
have determined the exact EQuiTemporal Surfaces (EQTSs) for the Gamma-Ray Burst
(GRB) afterglows. These surfaces are compared and contrasted to the ones
obtained, using approximate methods, by Panaitescu & Meszaros (1998), Sari
(1998), Granot et al. (1999).

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