Lognormal Properties of SGR 1806-20 and Implications for Other SGR Sources

K. J. Hurley; B. McBreen; M. Delaney; A. Britton

doi:10.1007/bf00658592

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arXiv · astro-ph/9508074

Lognormal Properties of SGR 1806-20 and Implications for Other SGR Sources

K. J. Hurley·B. McBreen·M. Delaney·A. Britton

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Abstract

The time interval between successive bursts from SGR 1806-20 and the intensity of these bursts are both consistent with lognormal distributions. Monte Carlo simulations of lognormal burst models with a range of distribution parameters have been investigated. The main conclusions are that while most sources like SGR 1806-20 should be detected in a time interval of 25 years, sources with means about 100 times longer have a probability of about 5\% of being detected in the same interval. A new breed of experiments that operate for long periods are required to search for sources with mean recurrence intervals much longer than SGR 1806-20.

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K. J. Hurley, B. McBreen, M. Delaney, A. Britton. 1995-08-24. Lognormal Properties of SGR 1806-20 and Implications for Other SGR Sources. https://doi.org/10.1007/bf00658592

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