Gamma-ray emission from pulsars and Hardee mechanism of e(+)e(-) production

Details Gamma-ray emission from pulsars and Hardee mechanism of e(+)e(-) production Gamma-ray emission from pulsars and Hardee mechanism of e(+)e(-) production

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...231l...7l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 2, May 1990, p. L7-L10. Research supported by the National Natural Sc

Astronomy and Astrophysics

Astronomy

16

Gamma Ray Astronomy, Pair Production, Pulsars, Crab Nebula, Luminosity, Radio Sources (Astronomy), Supernova 1987A

Scientific paper

Based on the Hardee (1977) mechanism of e(+)e(-) production at the magnetic axis by high energy gamma photons, the gamma-ray emission of pulsars is discussed. The criterion for radio pulsars appearing also as gamma-ray pulsars is given. Some characteristic quantities of radiation for the candidates of gamma-ray pulsars are calculated. The calculated luminosities for Crab and Vela pulsars are in agreement with the observed values. The discussion also covers the questions: does the newly discovered sub-milli-second optical pulsar in SN1987A be a gamma-ray pulsar?

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