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Lognormal properties of SGR 1806-20 and implications for other SGR sources (1995)

Hurley, K. J. ; McBreen, B. ; Delaney, M. ; [weitere]

Springer

Astrophysics and space science 231 (1995), S. 81-84

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Details

ISSN: 1572-946X

Schlagwort(e): Soft gamma repeaters ; Lognormal statistics ; Monte Carlo methods ; Pulsars ; Glitches

Quelle: Springer Online Journal Archives 1860-2000

Thema: Physik

Notizen: 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.

Materialart: Digitale Medien

URL: http://dx.doi.org/10.1007/BF00658592

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