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Continuous optical monitoring during the prompt emission of GRB 060111B
Ist Teil von
Astronomy and astrophysics (Berlin), 2006-06, Vol.451 (3), p.L39-L42
Ort / Verlag
Les Ulis: EDP Sciences
Erscheinungsjahr
2006
Link zum Volltext
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
Aims.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. Methods.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. Results.The optical emission was found to decay steadily from our first measure, 28 s 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.