θ-z test for QSO - galaxy physical association

dc.contributor.author	Sapre, A. K
dc.contributor.author	Nashine, R
dc.contributor.author	Mishra, V. D
dc.date.accessioned	2007-11-03T07:52:58Z
dc.date.available	2007-11-03T07:52:58Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 2, pp. 285 - 287	en
dc.identifier.uri	http://hdl.handle.net/2248/1949
dc.description.abstract	The 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.extent	234135 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999BASI...27..285S	en
dc.subject	QSO-galaxy	en
dc.subject	θ-z test	en
dc.title	θ-z test for QSO - galaxy physical association	en
dc.type	Article	en