Radio emission from Cyg X-3

Details Radio emission from Cyg X-3 Radio emission from Cyg X-3

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000basi...28..275a&link_type=abstract

Bulletin of the Astronomical Society of India, Vol. 28, p. 275-276 (2000)

Astronomy and Astrophysics

Astronomy

Scientific paper

The acceleration of high energy particles by a shock produced by the
passage of the secondary object in the binary system, through the wind
of the primary, is considered and is shown to be adequate to account for
the quiescent radio emission from Cyg X-3. A mechanism for inducing
large radio flares is outlined.

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