Studies of the gamma ray pulsar Geminga

Details Studies of the gamma ray pulsar Geminga Studies of the gamma ray pulsar Geminga

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..578z&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 578-582 (1997).

Computer Science

3

Pulsars, Neutron Stars, Ephemerides, Almanacs, And Calendars, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Gamma-Ray

Scientific paper

Ephemeris parameters of gamma ray pulsar Geminga have been revised using
EGRET. Timing and imaging analyses show that the majority emission of
Geminga are in phase region around the first peak in 10-30 MeV during
COMPTEL VP1. No turn off of spectrum appear at energies below 30 MeV.

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