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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1949
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dc.contributor.authorSapre, A. K-
dc.contributor.authorNashine, R-
dc.contributor.authorMishra, V. D-
dc.date.accessioned2007-11-03T07:52:58Z-
dc.date.available2007-11-03T07:52:58Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 2, pp. 285 - 287en
dc.identifier.urihttp://hdl.handle.net/2248/1949-
dc.description.abstractThe θ-z test devised by Burbidge et al, (1972, 1990) may serve as a powerful test to decide the reality or otherwise of the physical association hypothesis for the QSO-bright galaxy close pairs with discrepant redshifts. Recently, Burdidge (1996)has published a sample of 33 QSO-bright galaxy close pairs with discrepant redshifts as the best candidates for the physical association. In this paper, we have subjected this sample of 33 pairs to the θ-z test with a view to test the reality of the physical association of these pairs.en
dc.format.extent234135 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..285Sen
dc.subjectQSO-galaxyen
dc.subjectθ-z testen
dc.titleθ-z test for QSO - galaxy physical associationen
dc.typeArticleen
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