X-ray Tails Following Bursts from SGR 1900+14

Details X-ray Tails Following Bursts from SGR 1900+14 X-ray Tails Following Bursts from SGR 1900+14

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasb.conf..159w&link_type=abstract

"Pulsars, AXPs and SGRs observed with BeppoSAX and Other Observatories, Proceedings of the International Workshop held in Marsal

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During and following epochs of burst activity in Soft Gamma Repeaters (SGRs), we have observed brightening of their persistent X-ray emission. On four occasions thus far in SGR 1900+14, observed flux increases or tails of X-ray emission directly follow energetic bursts from the source. Here, I will summarize what we know about the spectral and temporal properties of these X-ray tails and draw comparisons between the four events. The changes in flux, source spectrum, pulsed fraction, and pulse shape will be presented. I will also briefly discuss efforts being made to understand their physical origin.

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