Young pulsar envelopes as gamma-ray sources

Details Young pulsar envelopes as gamma-ray sources Young pulsar envelopes as gamma-ray sources

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sval....3...79b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 3, Apr. 1977, p. 152-156.) Soviet Astronomy Letters, vol. 3, Mar.-Apr. 1977, p. 79-81.

Astronomy and Astrophysics

Astronomy

6

Gamma Ray Astronomy, Pulsars, Stellar Envelopes, Supernovae, Milky Way Galaxy, Neutrinos, Neutrons, Particle Acceleration, Protons

Scientific paper

The possibility of detecting gamma radiation from the dense supernova shell surrounding a young pulsar is investigated. The energy spectrum of gamma quanta emitted from a young pulsar by the mechanism of injection of protons from the pulsar into the expanding shell is calculated. Gamma quanta of energy above 100 MeV should be detectable by gamma-telescopes aboard satellites or balloons. Sources up to 15 Mpc distance from earth may be detected in this manner.

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