Interpretation of the pulsed gamma-ray emission from VELA

Details Interpretation of the pulsed gamma-ray emission from VELA Interpretation of the pulsed gamma-ray emission from VELA

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201l.117t&link_type=abstract

Astrophysical Journal, vol. 201, Nov. 1, 1975, pt. 2, p. L117-L120.

Astronomy and Astrophysics

Astronomy

13

Astronomical Models, Gamma Rays, Neutron Stars, Pulsars, Radio Emission, Supernova Remnants, Radiant Flux Density, Statistical Analysis, Synchrotron Radiation, X Ray Astronomy

Scientific paper

A model is proposed for the Vela pulsar in which the radio emission originates near the surface of the neutron star while the pulsed gamma-ray emission is produced by synchrotron radiation near the speed-of-light cylinder. This model can explain the energy flux, double pulse structure, and phase shift (with respect to the radio) of the gamma-ray emission, and offers approximate quantitative predictions for other X- and gamma-ray fluxes.

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