Geminga as a possible source of very-high-energy gamma rays

Details Geminga as a possible source of very-high-energy gamma rays Geminga as a possible source of very-high-energy gamma rays

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..434b&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 434; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 12, p. 1059-1065. I

Astronomy and Astrophysics

Astronomy

Emission Spectra, Gamma Ray Astronomy, High Energy Electrons, Neutron Stars, Electron Scattering, Light Curve, Positrons, Pulsar Magnetospheres, Relativistic Electron Beams, Stellar Radiation

Scientific paper

Lower limits on fluxes of very-high-energy gamma rays from Geminga are
estimated. This emission is generated by inverse Compton scattering of
relativistic electrons and positrons on thermal photons of the neutron
star surface. The light curve of Geminga in very-high-energy gamma rays
is discussed.

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