Gamma-ray emission from pulsars and SN 1987A sub-millisecond pulsars

Details Gamma-ray emission from pulsars and SN 1987A sub-millisecond pulsars Gamma-ray emission from pulsars and SN 1987A sub-millisecond pulsars

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990scsmp..33.1230l&link_type=abstract

Science in China, Series A - Mathematics, Physics, Astronomy and Technological Sciences (ISSN 1001-6511), vol. 33, Oct. 1990, p.

Mathematics

Logic

Electron-Positron Pairs, Gamma Rays, Pulsars, Radio Stars, Stellar Radiation, Supernova 1987A, Gauss Equation, Magnetic Dipoles, Radiation Absorption, Stellar Magnetic Fields, Synchrotron Radiation

Scientific paper

An evaluation is made of current understanding as to which radio pulsars could in addition be gamma-ray pulsars. After demonstrating the importance to the radio-pulsar gamma-ray pulsar relation of the Hardee mechanism of e(+)e(-) production at the magnetic axis by high-energy gamma photons, physical quantities are presented for several gamma-ray pulsar candidates. Attention is given to the possibility of gamma-ray emissions from the SN 1987A pulsar. It is suggested that, of more than 400 pulsars, no more than 21 are gamma-ray pulsar candidates; most gamma-ray photon fluxes are so weak as to be undetectable.

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