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Delayed Flashes from Counter Jets of Gamma Ray Bursts

Ryo Yamazaki·Kunihito Ioka·Takashi Nakamura
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Abstract

If X-ray flashes are due to the forward jet emissions from gamma ray bursts (GRBs) observed with large viewing angles, we show that a prompt emission from a counter jet should be observed as a delayed flash in the UV or optical band several hours to a day after the X-ray flash. Ultraviolet and Optical Telescope on Swift can observe the delayed flashes within ~13 Mpc, so that (double-sided) jets of GRBs may be directly confirmed. Since the event rate of delayed flashes detected by Swift may be as small as 6*10^{-5}events/yr, we require more sensitive detectors in future experiments.

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Ryo Yamazaki, Kunihito Ioka, Takashi Nakamura. 2003-03-13. Delayed Flashes from Counter Jets of Gamma Ray Bursts. https://doi.org/10.1086/375261

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