Physics
Scientific paper
May 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..266w&link_type=abstract
Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 266-270 (1998).
Physics
1
Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray
Scientific paper
We present here the results of the first search for submillisecond variability in gamma-ray bursts. We have examined 20 of the brightest BATSE bursts for isolated flares and for low amplitude fluctuations. We find that GRB970229 has a flare with a rise time of 200+/-30 μs and fall time of 300+/-50 μs. In addition we find all bursts to show activity on time scales of less than 30 ms. Typical bursts show activity on the time scale of a millisecond, while 30% of the burst show sub-millisecond activity. This result can be used to prove that the emission regions are patchy and that any spherical symmetry in the shell must be broken.
Schaefer Bradley E.
Walker Katharine C.
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