On the enhanced X-ray emission from SGR 1900+14 after the August 27th giant flare

Details On the enhanced X-ray emission from SGR 1900+14 after the August 27th giant flare On the enhanced X-ray emission from SGR 1900+14 after the August 27th giant flare

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004nuphs.132..530e&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 132, p. 530-535.

Physics

Nuclear Physics

Scientific paper

We show that the giant flares of soft gamma ray repeaters (E~1044 erg) can push the inner regions of a fall-back disk out to larger radii by radiation pressure, while matter remains bound to the system for plausible parameters. The subsequent relaxation of this pushed-back matter can account for the observed enhanced X-ray emission after the August 27th giant flare of SGR 1900+14.

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