BURST TAILS FROM SGR J1550-5418 OBSERVED WITH THE ROSSI X-RAY TIMING EXPLORER

ABSTRACT We present the results of our extensive search using the Bayesian block method for long tails following short bursts from a magnetar, SGR J1550-5418, over all RXTE observations of the source. We identified four bursts with extended tails, most of which occurred during its 2009 burst active...

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Bibliographic Details
Published in:The Astrophysical journal Vol. 807; no. 1; pp. 1 - 9
Main Authors: Mu, Sinem a maz, Göğü, Ersin, Kaneko, Yuki, Chakraborty, Manoneeta, Ayd n, Berk
Format: Journal Article
Language:English
Published: United States The American Astronomical Society 01-07-2015
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Summary:ABSTRACT We present the results of our extensive search using the Bayesian block method for long tails following short bursts from a magnetar, SGR J1550-5418, over all RXTE observations of the source. We identified four bursts with extended tails, most of which occurred during its 2009 burst active episode. The durations of tails range between ∼13 s and over 3 ks, which are much longer than the typical duration of bursts. We performed detailed spectral and temporal analyses of the burst tails. We find that the spectra of three tails show a thermal nature with a trend of cooling throughout the tail. We compare the results of our investigations with the properties of four other extended tails detected from SGR 1900+14 and SGR 1806-20 and suggest a scenario for the origin of the tail in the framework of the magnetar model.
Bibliography:ApJ98653
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ISSN:0004-637X
1538-4357
1538-4357
DOI:10.1088/0004-637X/807/1/42