SAS 2 observation of pulsed high-energy gamma radiation from Geminga

Details SAS 2 observation of pulsed high-energy gamma radiation from Geminga SAS 2 observation of pulsed high-energy gamma radiation from Geminga

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...401l..23m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 401, no. 1, p. L23-L26.

Astronomy and Astrophysics

Astronomy

39

Gamma Ray Astronomy, Pulsars, Satellite Observation, Gamma Ray Telescopes, Particle Acceleration

Scientific paper

Following the detection of pulsed X-rays and gamma rays from Geminga, the 1972-1973 SAS 2 data which first revealed this source have been reanalyzed. The 237 ms periodicity is visible in those observations. The phase of the SAS 2 periodicity is consistent with that of COS B suggesting that the gamma-ray data allow an accounting for every revolution of the Geminga pulsar between 1972 and 1982.

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