Radio emission from Cyg X-3

dc.contributor.author	Apparao, K. M. V
dc.date.accessioned	2008-02-29T11:17:54Z
dc.date.available	2008-02-29T11:17:54Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 275 - 276	en
dc.identifier.uri	http://hdl.handle.net/2248/2101
dc.description.abstract	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.	en
dc.format.extent	144451 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000BASI...28..275A	en
dc.subject	Radio emission	en
dc.subject	Binary system	en
dc.title	Radio emission from Cyg X-3	en
dc.type	Article	en