Issue |
A&A
Volume 437, Number 2, July II 2005
|
|
---|---|---|
Page(s) | L23 - L25 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:200500125 | |
Published online | 21 June 2005 |
Letter to the Editor
Early BVR
I
imaging and the discovery of the optical afterglow of GRB 041218
Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama-cho, Toyonaka, Osaka 560-0043, Japan e-mail: torii@ess.sci.osaka-u.ac.jp
Received:
16
March
2005
Accepted:
3
May
2005
We report early imaging of the INTEGRAL GRB 041218. The observation started 129 s after the burst and a sequence
of exposures in V, Rc, Ic, and B bands were
repeated. The optical afterglow is detected in Rc and
bands while it was not detected in B and V. We find that the
early afterglow deviates from a single power law decay and identify
two characteristic timescales (breaks). Such breaks are theoretically
expected from synchrotron cooling in the relativistic fireball (Sari
et al. 1998, ApJ, 497, L17) and we crudely constrain the physical condition of the
relativistic shock.
Key words: gamma rays: bursts
© ESO, 2005
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