Searches for gamma ray emission from radio pulsars

Details Searches for gamma ray emission from radio pulsars Searches for gamma ray emission from radio pulsars

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..220t&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 1, Oct. 1983, p. 220-223.

Astronomy and Astrophysics

Astrophysics

8

Emission Spectra, Gamma Rays, Pulsars, Gamma Ray Telescopes, Sas-2, Stellar Luminosity

Scientific paper

Searches have been made for pulsed high energy (E > 35 MeV) γ-radiation from 43 pulsars using the SAS-2 data base and radio parameters which became available after the previous search of Ögelman et al. (1976). No positive results were found, and the upper limits are consistent with the concept that γ-ray production efficiency increases with increasing apparent age. Two limits from the Ögelman et al. (1976) search, however suggest that efficiency cannot be a simple function of apparent age beyond 106 yr.

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