Gamma ray bursts: Current status of observations and theory

Details Gamma ray bursts: Current status of observations and theory Gamma ray bursts: Current status of observations and theory

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3071..217m&link_type=abstract

In NASA, Goddard Space Flight Center, The Energetic Gamma-Ray Experiment Telescope (EGRET) Science Symposium p 217-231 (SEE N90-

Physics

Gamma Ray Bursts, Gamma Rays, Magnetic Stars, Neutron Stars, Spectrum Analysis, Energy Spectra, Gamma Ray Spectra

Scientific paper

Gamma-ray bursts display a wide range of temporal and spectral characteristics, but typically last several seconds and emit most of their energy in the low-energy gamma-ray region. The burst sources appear to be isotropically distributed on the sky. Several lines of evidence suggest magnetic neutron stars as sources for bursts. A variety of energy sources and emission mechanisms were proposed.

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