Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..126a&link_type=abstract
Soviet Astronomy Letters, Vol. 18, p. 126; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 4, April 1992, p. 31
Astronomy and Astrophysics
Astronomy
Gamma Ray Astronomy, Light Curve, Pulsars, Gamma Ray Telescopes, Stellar Radiation
Scientific paper
The Vela pulsar PSR 0833 - 45 was observed with the Gamma-1 gamma-ray telescope in summer 1990 and spring 1991. Data of recent radio measurements are used to construct light curves of the pulsar and perform a preliminary temporal analysis for gamma-ray energy above 100 MeV. In particular, attention is given to the positions of main light-curve features with respect to the radio phase and also to the hypothesis of the variability of the intensity of the pulsed emission on the basis of data of two observations separated by a six-month interval. These results are compared to findings obtained by the COS-B group.
Afanasyev V. G.
Akimov Vladlen V.
Belaousov A. S.
Blokhintsev I. D.
Galper Arkady M.
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