9.22-MILLISECOND Very High Energy Gamma-Ray Pulsar in CYGNUS-X-3

Details 9.22-MILLISECOND Very High Energy Gamma-Ray Pulsar in CYGNUS-X-3 9.22-MILLISECOND Very High Energy Gamma-Ray Pulsar in CYGNUS-X-3

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1508....1z&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1508/SEP, P. 1, 1987

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Observations of very high-energy gamma-ray quanta from Cyg X-3 using
Cherenkov technique and precise arriving time of light pulses were made
at the Crimean Astrophysical Observatory during September 1978. The
analysis shows that there exists 9.22 ms periodicity in Cherenkov
pulses.

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