Ultrahigh-Energy Gamma-Ray Emission from the Geminga Pulsar

Details Ultrahigh-Energy Gamma-Ray Emission from the Geminga Pulsar Ultrahigh-Energy Gamma-Ray Emission from the Geminga Pulsar

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001astl...27..228n&link_type=abstract

Astronomy Letters, vol. 27, p. 228-232 (2001)

Astronomy and Astrophysics

Astronomy

6

Pulsars, Ground-Based Gamma-Ray Astronomy, Gamma-Ray Photons

Scientific paper

In 1996-1997, the Geminga pulsar was observed at the Crimean Astrophysical Observatory with a ground-based gamma-ray telescope. An analysis of the observational data suggests that this object is a source of ultrahigh-energy gamma rays. An analysis of the temporal distribution of gamma-ray photons by an epoch-folding technique reveals a periodicity in the gamma-ray emission with a period of 0.237 s.

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