The 10-30 MeV gamma-ray emission of the Geminga pulsar

Details The 10-30 MeV gamma-ray emission of the Geminga pulsar The 10-30 MeV gamma-ray emission of the Geminga pulsar

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acasn..38..331z&link_type=abstract

Acta Astronomica Sinica, vol. 38, p. 331

Astronomy and Astrophysics

Astronomy

Gamma Rays, Pulsars, Gamma Ray Astronomy, Satellite Observation, Demodulation

Scientific paper

The absolute phases of Geminga observed by COMPTEL Obs. 1 and EGRET Obs. 1 have been compared. The phase-resolved imaging results obtained by a direct demodulation method show that the gamma-ray emission of Geminga in the 10-30 MeV range may exist mainly in the peak phase 1 region. This result conforms to the variational trend of intensity ratio P2/P1 with energy.

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