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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/945
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dc.contributor.authorRajamohan, R-
dc.contributor.authorBhattacharyya, J. C-
dc.contributor.authorSubramanian, V-
dc.contributor.authorKuppuswamy, K-
dc.date.accessioned2006-04-11T08:24:35Z-
dc.date.available2006-04-11T08:24:35Z-
dc.date.issued1988-12-
dc.identifier.citationBASI, Vol. 16, No. 4, pp. 139-144en
dc.identifier.urihttp://hdl.handle.net/2248/945-
dc.description.abstractSchmidt plates of the old open galactic cluster M67 were obtained on twelve nights to find the most probable variables in the cluster. The Sabattier technique was used to derive the magnitudes of the cluster members. The most probable variable stars in this cluster determined by this method are listed.en
dc.format.extent413983 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indianen
dc.subjectOpen clusteren
dc.subjectVariable starsen
dc.titleVariable stars in the old galactic cluster M67en
dc.typeArticleen
Appears in Collections:BASI Publications
J.C.Bhattacharyya (1982 - 1990)

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