Gamma-ray burst spectroscopy

Details Gamma-ray burst spectroscopy Gamma-ray burst spectroscopy

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..170..258h&link_type=abstract

AIP Conference Proceedings, Volume 170, pp. 258-264 (1988).

Statistics

2

Scientific paper

The statistics and physical properties of gamma ray burst spectral features are presented, following a brief review of early theoretical predictions of, and experimental searches for, such emission. The ~100 observations of 50 keV absorption and 400 keV emission features constitute the largest data base on neutron star lines. Although the statistical significance of individual observations is often weak, and interpretation of these features as cyclotron absorption and annihilation radiation poses some theoretical problems, it is clear that future observations may have far-reaching implications.

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