Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...128..245b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 128, no. 1, Nov. 1983, p. 245-251.
Astronomy and Astrophysics
Astrophysics
288
Cos-B Satellite, Gamma Rays, Pulsars, Stellar Radiation, Radio Emission
Scientific paper
Pulsed gamma-ray emission from radio pulsars has been sought in a study of pulsar parameters for 145 radio observations, contemporary with gamma-ray observations, by the COS-B spacecraft. No signal has been detected in the 50 MeV-2 GeV energy range of the study, either globally or from individual pulsars. These results indicate that the average product of the conversion efficiency from the pulsar braking power into gamma-rays, and the pulsar moment of inertia, cannot exceed 6 x 10 to the 43rd g/sq cm, for pulsar ages greater than 40,000 years. This implies that the contribution of old pulsars to the observed galactic gamma-ray emission is less than 5 percent for gamma-ray energies greater than 50 MeV.
Bennett Kevin
Bignami Giovanni F.
Bloemen Johannes Bernardus Gerhardus Maria
Boriakoff Valentin
Buccheri Rosolino
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