On evolutionary models of radio sources

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4217

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DC Field	Value	Language
dc.contributor.author	Swarup, G.	-
dc.contributor.author	Subrahmanya, C.R.	-
dc.contributor.author	Kapahi, V.K.	-
dc.date.accessioned	2011-12-15T05:42:14Z	-
dc.date.available	2011-12-15T05:42:14Z	-
dc.date.issued	1982	-
dc.identifier.citation	In: Astrophysical cosmology; Proceedings of the Study Week on Cosmology and Fundamental Physics, Vatican City State, September 28-October 2, 1981. (A82-42276 21-90) Vatican City State, Pontificia Academia Scientiarum, 1982, p. 383-390	en
dc.identifier.uri	http://hdl.handle.net/2289/4217	-
dc.description	Restricted Access.	en
dc.description.abstract	Evolutionary effects in the properties of extragalactic radio sources are known to dominate the geometrical effects of reasonable world models. Two aspects of the evolution of radio sources are considered, namely the use of optical identification data to constrain possible changes in the radio luminosity function with epoch and the evidence for evolution in the linear sizes of double radio sources.	en
dc.language.iso	en	en
dc.publisher	Pontificia Academia Scientiarum	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1982ac...proc..383S	en
dc.rights	1982 Pontificia Academia Scientiarum	en
dc.subject	Astronomical Models	en
dc.subject	Cosmology	en
dc.subject	Radio Sources (Astronomy)	en
dc.subject	Evolution (Development)	en
dc.subject	Extragalactic Radio Sources	en
dc.subject	Flux Density	en
dc.subject	Luminosity	en
dc.title	On evolutionary models of radio sources	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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