The spectroscopy of classical gamma-ray bursts

Details The spectroscopy of classical gamma-ray bursts The spectroscopy of classical gamma-ray bursts

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..366..206b&link_type=abstract

High velocity neutron stars and gamma-ray bursts. AIP Conference Proceedings, Volume 366, pp. 206-210 (1996).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The continua of classical gamma ray bursts observed by the CGRO instruments are well described by a simple four parameter model between 10 keV and 100 MeV. Additional components above and below this energy range are sometimes present; the high energy component persisted in one burst for more than 90 minutes after the lower energy emission. The spectral hardness generally increases and decreases with the count rate, with a superimposed hard-to-soft trend within and between emission spikes. Finally, no absorption lines have been detected in the BATSE spectra, although the apparent discrepancy between previous detections and the absence of a BATSE detection is not yet compelling.

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