Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-04-04
Astronomy and Astrophysics
Astrophysics
Scientific paper
10.1051/0004-6361:20065158
We present the time-resolved optical emission of GRB 060111B during its prompt phase, measured with the TAROT robotic observatory. This is the first time that the optical emission from a gamma-ray burst has been continuously monitored with a temporal resolution of a few seconds during the prompt gamma-ray phase. The temporal evolution of the prompt optical emission at the level of several seconds is used to provide a clue to the origin of this emission. The optical emission was found to decay steadily from our first measure, 28s after the trigger, in contrast to the gamma-ray emission, which exhibits strong variability at the same time. This behaviour strongly suggests that the optical emission is due to the reverse shock.
Atteia Jean-Luc
Behrend Raoul
Boer Michel
Damerdji Yassine
Gendre Bruce
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