The very early optical afterglow of GRBs, revealing the nature of the ejecta

Details The very early optical afterglow of GRBs, revealing the nature of the ejecta The very early optical afterglow of GRBs, revealing the nature of the ejecta

2005-03-08

arxiv.org/abs/astro-ph/0503194v2

eConf C041213:2205,2004

Astronomy and Astrophysics

Astrophysics

To appear in Proc. of 22nd Texas Symposium on Relativistic Astrophysics, Stanford Univ., December 2004, (PSN 2205), 5 pages, L

Scientific paper

We show that if the GRB ejecta itself is magnetized or neutron-rich, the very
early afterglow of GRBs is very different from that powered by a pure ion
fireball. In the Swift era, with the well monitored early afterglow data, we
can potentially diagnose the ejecta composition and reveal the nature of the
central GRB engine.

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