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A ug 1 99 5 Lognormal Properties of SGR 1806-20 and Implications for Other SGR Sources
| Content Provider | Semantic Scholar |
|---|---|
| Author | McBreen, Brian Delaney, Michelle Britton, Andrea |
| Copyright Year | 1995 |
| 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. |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | http://arxiv.org/pdf/astro-ph/9508074v2.pdf |
| Language | English |
| Access Restriction | Open |
| Subject Keyword | Breeding Experiment Leucaena pulverulenta Monte Carlo method Ninety Nine Samsung SGR-A1 Simulation |
| Content Type | Text |
| Resource Type | Article |
