Parametric decay instability in 3C 273

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4774

Full metadata record

DC Field	Value	Language
dc.contributor.author	Gangadhara, R. T	-
dc.contributor.author	Krishan, V	-
dc.date.accessioned	2009-08-28T14:55:57Z	-
dc.date.available	2009-08-28T14:55:57Z	-
dc.date.issued	1991	-
dc.identifier.citation	Miller, Richard H and Wiita, Paul J. eds., Variability of active galactic nuclei., Georgia State University Conference on Variability of Active Galactic Nuclei, May 2 - 4,1990. pp. 190 - 193	en
dc.identifier.isbn	0-521-41295-1	-
dc.identifier.uri	http://hdl.handle.net/2248/4774	-
dc.description.abstract	The parametric decay instability (PDI) causes anomalous absorption of strong electromagnetic (e.m) radiation under specific conditions of energy and momentum conservation. It is shown that in the source 3C 273, the conditions are conducive to the excitation of PDI. This process also contribute towards the absorption of 21-cm radiation	-
dc.language.iso	en	en
dc.publisher	Cambridge University Press	en
dc.subject	Parametric Decay	en
dc.subject	Instability in 3C 273	en
dc.title	Parametric decay instability in 3C 273	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Parametric Decay Instability		55.7 kB	Adobe PDF	View/Open

DSpace JSPUI