Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/2101
Title: | Radio emission from Cyg X-3 |
Authors: | Apparao, K. M. V |
Keywords: | Radio emission Binary system |
Issue Date: | 2000 |
Publisher: | Astronomical Society of India |
Citation: | BASI, Vol. 28, No. 2, pp. 275 - 276 |
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. |
URI: | http://hdl.handle.net/2248/2101 |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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apparao_1.pdf | 141.07 kB | Adobe PDF | View/Open |
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