Gamma rays of 1-30 MeV from the VELA Pulsar PSR 0833-45

Details Gamma rays of 1-30 MeV from the VELA Pulsar PSR 0833-45 Gamma rays of 1-30 MeV from the VELA Pulsar PSR 0833-45

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9...37t&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Physics

Gamma Ray Spectra, Pulsars, Radiant Flux Density, Stellar Radiation, Stellar Spectrophotometry, Photon Density, Spectral Energy Distribution

Scientific paper

Results are reported for observations of gamma rays of 1-30 MeV from the Vela Pulsar PSR 0833 - 45 carried out with the UCR double scatter gamma ray telescope on a balloon launched from Alice Springs, Australia on November 10, 1981. An integrated flux of (5.3 + or - 1.3) x 10 to the -4th photons/sq cm/s is found for the Vela region above 2 MeV. This value, together with those for the energy intervals of 2-4, 4-7, and 7-15 MeV are in reasonable agreement with the power law found by COS-B at energies above 50 MeV. A sky contour map of the fluxes is shown.

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