High-energy cosmic gamma rays in the Southern Hemisphere

Details High-energy cosmic gamma rays in the Southern Hemisphere High-energy cosmic gamma rays in the Southern Hemisphere

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974csgr.conf..265f&link_type=abstract

In ESRO The Context and Status of Gamma Ray Astronomy p 265-271 (SEE N75-25813 16-93)

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Galactic Radiation, Gamma Rays, Magellanic Clouds, Point Sources, Southern Hemisphere, Balloon Sounding, Cosmic Rays, Emission Spectra, Oso-3, Oso-7, Sas, Satellite Observation, X Ray Sources

Scientific paper

Pulsed 20 MeV gamma rays from the Vela pulsar, PSR 0833-45, were detected on a balloon flight from Longreach, Queensland, using a spark chamber pointed at 35 deg south of zenith. The time average flux was of 0.000015 MeV/sq cm sec MeV. Evidence is also seen for gamma radiation from the Large Magellanic Cloud. A comparison with OSO-7 ray surveys indicates that at least some of the galactic plane gamma rays are from point sources.

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