Cygnus X-3 - a pulsar with period of 4.8 H

Details Cygnus X-3 - a pulsar with period of 4.8 H Cygnus X-3 - a pulsar with period of 4.8 H

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pazh....2..334s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 2, July 1976, p. 334-337. In Russian.

Astronomy and Astrophysics

Astronomy

4

Binary Stars, Pulsars, Stellar Motions, X Ray Sources, Infrared Stars, Orbital Elements, Stellar Temperature, Supergiant Stars

Scientific paper

It is hypothesized that the X-ray source Cyg X-3 is a long-period accreting pulsar and along with a red supergiant forms a binary system with orbital period of several years. Interpretation of the normal component as a red supergiant with low surface temperature (less than 3000 K) and with a hot spot can account for the observed infrared flux from Cyg X-3.

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