Gamma-ray spectra expected from pulsars

Details Gamma-ray spectra expected from pulsars Gamma-ray spectra expected from pulsars

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....71...51m&link_type=abstract

Astronomy and Astrophysics, vol. 71, no. 1-2, Jan. 1979, p. 51-54.

Astronomy and Astrophysics

Astrophysics

10

Gamma Rays, Pulsars, Stellar Models, Stellar Spectra, X Ray Spectra, Astronomical Catalogs, Pair Production, Photoabsorption, Synchrotron Radiation

Scientific paper

A grid of gamma-ray spectra of pulsars is calculated according to a model where the primary radiation consists of curvature photons; photon absorption by magnetic pair production and secondary synchrotron emission are allowed for. The pulsar period, the initial Lorentz factor of the primary particles, and the surface magnetic field have been taken as free parameters, and their influence on the spectral shape is shown and discussed. Hardness ratios and radiation efficiencies are also given. Observational implications are suggested for the unidentified gamma-ray sources.

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