Radio and infrared flares in CYG X-3

Details Radio and infrared flares in CYG X-3 Radio and infrared flares in CYG X-3

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.133..229a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 133, no. 2, 1987, p. 229-231.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Infrared Spectra, Plasma-Electromagnetic Interaction, Radio Spectra, Stellar Flares, X Ray Sources, Gamma Rays, Kepler Laws, Pulsars

Scientific paper

The observed radio and infrared flares in Cyg X-3 are explained as due
to interaction of X-rays and high-energy gamma-rays with clumps of
matter in a cocoon around the object. The observed repetitive period of
the radio flares is explained as the beat period between the 4.8 hr
periodicity and the Keplerian period of matter in the cocoon.

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