Time variations of high energy gamma emission of VELA Pulsar observed by GAMMA-1 telescope

Details Time variations of high energy gamma emission of VELA Pulsar observed by GAMMA-1 telescope Time variations of high energy gamma emission of VELA Pulsar observed by GAMMA-1 telescope

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..657a&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 13, no. 12, p. (12)657-(12)664

Astronomy and Astrophysics

Astronomy

Energy Spectra, Gamma Ray Astronomy, Light Curve, Pulsars, Radiant Flux Density, Variations, Astronomical Satellites, Gamma Ray Telescopes

Scientific paper

Two observations of the Vela Pulsar in the energy range 50-5000 MeV performed with the GAMMA-1 telescope in 1990 and 1991 allowed us to study time variability of the pulsar light curve and energy spectra. The light curve for Egamma greater than 50 MeV shows definite variations in the first interpeak phase interval. The energy spectra of the two main peaks and first interpreak in the lightcurve vary significantly below 200 MeV.

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