We study the temporal and coarse spectral properties of 268 bursts from SGR 1806-20 and 679 bursts from SGR 1900+14, all observed with the Rossi X-Ray Timing Explorer /Proportional Counter Array. Hardness ratios and temporal parameters, such as T 90 durations and τ 90 emission times are determined for these bursts. We find a lognormal distribution of burst durations, ranging over more than 2 orders of magnitude: T 90 ~ 10 -2 to ≳1 s, with a peak at ~0.1 s. The burst light curves tend to be asymmetrical, with more than half of all events showing rise times t r < 0.3 T 90 . We find that there exists a correlation between the duration and fluence of bursts from both sources. We also find a significant anticorrelation between hardness ratio and fluence for SGR 1806-20 bursts and a marginal anticorrelation for SGR 1900+14 events. Finally, we discuss possible physical implications of these results within the framework of the magnetar model.
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Ersin Göğüş (2001) studied this question.
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