COS-B upper limits on gamma-ray emission from radio pulsars

Details COS-B upper limits on gamma-ray emission from radio pulsars COS-B upper limits on gamma-ray emission from radio pulsars

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9...49b&link_type=abstract

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

Physics

Emission Spectra, Gamma Ray Spectra, Pulsars, Stellar Evolution, Cos-B Satellite, Radio Spectra, Stellar Luminosity, Stellar Spectrophotometry

Scientific paper

The authors report on the results of a search for pulsed gamma-ray emission from old radio pulsars in the COS-B data in the energy range 50 MeV to 2 GeV. The analysis has been done by using either pulsar parameters obtained in simultaneous radio and gamma-ray observations or parameters which could be reliably derived by interpolation from radio observations spanning the COS-B observations.

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