Multiple imaging of quasars by galaxies and clusters

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2408

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DC Field	Value	Language
dc.contributor.author	Narayan, R.	-
dc.contributor.author	Blandford, R.	-
dc.contributor.author	Nityananda, R.	-
dc.date.accessioned	2007-05-25T08:16:17Z	-
dc.date.available	2007-05-25T08:16:17Z	-
dc.date.issued	1984-07-12	-
dc.identifier.citation	Nature, 1984, Vol.310, p112-115	en
dc.identifier.issn	0028-0836	-
dc.identifier.issn	1476-4687 (online)	-
dc.identifier.uri	http://hdl.handle.net/2289/2408	-
dc.description	Restricted Access.	en
dc.description.abstract	Multiply-imaged quasars have generally been explained as a combination of gravitational lensing by galaxies and magnification by clusters. The observational difficulties with this view suggest that some such quasars may be more naturally interpreted as images split by the cores of very rich clusters. The observational distinctions between the two models are discussed.	en
dc.format.extent	344881 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Nature Publishing Group	en
dc.relation.uri	http://dx.doi.org/10.1038/310112a0	en
dc.rights	1984 Nature Publishing Group	en
dc.title	Multiple imaging of quasars by galaxies and clusters	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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