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- W3099353462 abstract "We analyzed temporal and spectral properties, focusing on the short bursts, for three anomalous X-ray pulsars (AXPs) and soft gamma repeaters (SGRs), including SGR 1806-20, 1E 1048-5937 and SGR 0501+4516. Using the data from XMM-Newton, we located the short bursts by Bayesian blocks algorithm. The short bursts' duration distributions for three sources were fitted by two lognormal functions. The spectra of shorter bursts ($< 0.2~rm s$) and longer bursts ($geq 0.2~rm s$) can be well fitted in two blackbody components model or optically thin thermal bremsstrahlung model for SGR 0501+4516. We also found that there is a positive correlation between the burst luminosity and the persistent luminosity with a power law index $gamma = 1.23 pm 0.18 $. The energy ratio of this persistent emission to the time averaged short bursts is in the range of $10 - 10^3$, being comparable to the case in Type I X-ray burst." @default.
- W3099353462 created "2020-11-23" @default.
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- W3099353462 date "2015-03-01" @default.
- W3099353462 modified "2023-10-16" @default.
- W3099353462 title "The Short Bursts in SGR 1806−20, 1E 1048−5937, and SGR 0501+4516" @default.
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- W3099353462 doi "https://doi.org/10.1086/680484" @default.
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