Radio emission from Cyg X-3

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DC Field	Value	Language
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
Appears in Collections:	BASI Publications

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