Properties of the 1979 March 5 gamma-ray burst source

Details Properties of the 1979 March 5 gamma-ray burst source Properties of the 1979 March 5 gamma-ray burst source

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acaps..10...36g&link_type=abstract

(Acta Astrophysica Sinica, vol. 10, no. 1, 1990, p. 36-41) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 14, June 19

Astronomy and Astrophysics

Astrophysics

Annihilation Reactions, Gamma Ray Bursts, Spectrum Analysis, Bremsstrahlung, Interstellar Magnetic Fields, Radiation Sources

Scientific paper

The observed spectrum of the March 5, 1979 gamma-ray burst is fitted with a combination of thermal-synchrotron and pair-annihilation spectra; then, combined with some other observed data, it is found that the distance of the burst source cannot be greater than 2.2 kpc, so the source is not located in the SNR N49 of the LMC. The magnetic field of the source is in the range 150-1500 GG; the synchrotron radiation region has thickness 0.05-2.80 cm; and the two-photon annihilation region has thickness 80-240 cm.

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