Log-Normal Distributions in Gamma-Ray Burst Time Histories
arXiv:astro-ph/9607131 · doi:10.1086/310275
Abstract
We propose a new, simple but powerful algorithm to analyze the gamma-ray burst temporal structures based on identifying non-statistical variations (``peaks'') in the time histories. Detailed analyses of the bursts from the third BATSE catalog show that bursts have more than 20 peaks individually. Upon identifying most of the peaks in those bursts, we show that the peak fluence and peak interval distributions within each burst are consistent with log-normal distributions. Furthermore, we show that Gaussian (in linear space) and power-law distributions for peak fluences are ruled out, as is the Poisson distribution for peak intervals.
4 figures, AASTeX, to appear in ApJ Letters
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