Pulsed gamma-rays from PSR 1951 + 32

Details Pulsed gamma-rays from PSR 1951 + 32 Pulsed gamma-rays from PSR 1951 + 32

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acaps...9..298l&link_type=abstract

(Acta Astrophysica Sinica, vol. 9, no. 4, 1989, p. 298-304) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 14, March

Astronomy and Astrophysics

Astronomy

1

Gamma Ray Astronomy, Photon Density, Pulsars, Luminous Intensity, Radio Astronomy, Temporal Distribution

Scientific paper

In a previous paper significant evidence was obtained statistically for a 39-ms period in the COS-B data of 30-5000 MeV gamma rays in the direction of PSR 1951 + 32. Most of the gamma photons from PSR 1951 + 32 are pulsed and concentrated in a narrow interval of phase. The partial distribution of gamma ray intensity has been examined in the region around the pulsar and estimated the integrated flux to be 4.1 x 10 to the -7th ph/sq cm s above 100 MeV and 8.2 x 10 to the -8th ph/sq cm s above 300 MeV.

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