Gamma-ray emission from pulsars

Details Gamma-ray emission from pulsars Gamma-ray emission from pulsars

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223..147z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 147-153. Research supported by the National Natura

Astronomy and Astrophysics

Astronomy

18

Emission Spectra, Gamma Ray Astronomy, Pulsars, Astronomical Models, Crab Nebula, Luminosity, Statistical Analysis

Scientific paper

The mechanism of gamma-ray emission from pulsars is presently discussed on the basis of the Rudermann-Sutherland model, according to which the curvature radiation of typical energy around E(c) will be emitted by first-generation electrons after their effective accelerations within the polar gap. Attention is given to the criterion for the division of all pulsars into those solely observable as radio pulsars (PR type), and those which are in addition observable as gamma-ray pulsars (GR type).

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