Gamma-ray astronomy at the highest energies

Details Gamma-ray astronomy at the highest energies Gamma-ray astronomy at the highest energies

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nimpa.280..349w&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 280, Issue 2-3, p. 349-357.

Physics

Scientific paper

One of the major astronomical discoveries of the past decade has been the detection of gamma rays of energy in excess of 0.1 TeV from a variety of galactic sources. These detections were made with ground-based telescopes using the earth's atmosphere as the detecting medium. The sources detected include the Crab Nebula (a 940 year old supernova remnant), some millisecond radio pulsars (rotating neutron stars), and binary X-ray sources (close-binaries systems containing accreting neutron stars).

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