Possible discovery of three gamma-ray pulsars

Details Possible discovery of three gamma-ray pulsars Possible discovery of three gamma-ray pulsars

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.201..113m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 201, no. 1, p. 113-119.

Astronomy and Astrophysics

Astronomy

7

Cos-B Satellite, Gamma Ray Astronomy, Pulsars, Spaceborne Astronomy, Crab Nebula, Fourier Analysis, Radio Astronomy

Scientific paper

Data obtained by COS-B satellite were analyzed with the purpose of searching for gamma-ray pulsar emission, using two common methods, the Fourier analysis and the folding method. Three new gamma-ray pulsars were discovered: 0656 + 14, 0950 + 08, and 1822 - 09. Their light curves and other related features are presented. Among the three new gamma-ray pulsars, the PSR 0656 + 14 is the most significant one.

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