Magnitudes and colours of some members of the Perseus Cluster

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1981

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DC Field	Value	Language
dc.contributor.author	Bappu, M. K. V	-
dc.date.accessioned	2007-11-28T10:19:53Z	-
dc.date.available	2007-11-28T10:19:53Z	-
dc.date.issued	1954	-
dc.identifier.citation	Monthly Notices of Royal Astronomical Society, Vol. 114, No. 6, pp. 687-691	en
dc.identifier.uri	http://hdl.handle.net/2248/1981	-
dc.description.abstract	Photoelectric colours and magnitudes have been determined for twenty-five stars considered to be members of the moving cluster in Perseus. A distance modulus of 6m.83, corresponding to a distance of 230 ps, has been derived. This value is nearly twice the value of 120 ps derived by Miss Roman and Morgan from the upsilon component of proper motion.	en
dc.format.extent	344049 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1954MNRAS.114..687V	en
dc.subject	Photoelectric Colours and Magnitudes	en
dc.subject	Perseus Cluster	en
dc.subject	M.K.V. Bappu	en
dc.title	Magnitudes and colours of some members of the Perseus Cluster	en
dc.type	Article	en
Appears in Collections:	M.K. Vainu Bappu ( 1960 - 1982 )

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