Observations of gamma-ray burst spectra between 5 keV and 100 MeV

Details Observations of gamma-ray burst spectra between 5 keV and 100 MeV Observations of gamma-ray burst spectra between 5 keV and 100 MeV

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97...43b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 1, p. 43-48.

Astronomy and Astrophysics

Astronomy

15

Gamma Ray Astronomy, Gamma Ray Bursts, Absorption Spectra, Astronomical Spectroscopy, Emission Spectra

Scientific paper

The Franco-Soviet Lilas, Apex (Phobos mission), and Phebus (Granat satellite) experiments allow spectral observations of cosmic gamma-ray bursts over a very broad energy range from 5 keV up to 100 MeV. We present here typical results on continuum shapes, multiple absorption dips at low-energy (less than 100 keV), emission features around 500 keV, and spectral breaks at about 1 MeV. These observations are discussed in the framework of a highly-mgnetized emission source.

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