Search for a 12.59 MS pulsar in Cygnus X-3

Details Search for a 12.59 MS pulsar in Cygnus X-3 Search for a 12.59 MS pulsar in Cygnus X-3

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...211l...1f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 211, no. 1, Feb. 1989, p. L1-L4. Research supported by the National Board of S

Astronomy and Astrophysics

Astronomy

16

Gamma Ray Astronomy, Pulsars, X Ray Binaries, Cygnus Constellation, Emission Spectra, Light Curve, Power Spectra

Scientific paper

Observations made on Cygnus X-3 with the Whipple Observatory's 10-m imaging telescope between April 1983 and November 1986 were examined for the evidence of a 12.59 msec pulsar, the presence of which was reported by Chadwick et al. (1985). The data base was analyzed to find evidence of periodic emission of gamma-rays from Cygnus X-3 for periods between 12.586 and 12.596 msec for episodes of 8-min duration which cover the 4.8-h phase range from 0.55 to 0.70. During this period of time, no statistically significant pulsations were found within the period range examined.

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