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

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7528997t&link_type=abstract

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Gamma Rays, Neutron Stars, Pulsars, Pulsed Radiation, Astronomical Models, Photointerpretation, Radio Emission

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-ray and gamma-ray fluxes.

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