Computer Science
Scientific paper
Apr 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..366...68f&link_type=abstract
High velocity neutron stars and gamma-ray bursts. AIP Conference Proceedings, Volume 366, pp. 68-72 (1996).
Computer Science
Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray
Scientific paper
The March 5th, 1979 transient occurred on a source which is also a soft gamma repeater (SGR). A new analysis of the March 5th spectrum has shown that it is similar to a classic gamma-ray burst (no SGR-like component). Here we show that the variation in hardness within the initial peak is similar to that found in short, classic gamma-ray bursts. An analysis of the risetime of the peak shows that the best limit that can be put on it is <=1 ms rather than the previously reported 0.2 ms. Classic gamma-ray bursts have shown risetimes the order of 2 ms.
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