Variable stars in the old galactic cluster M67

dc.contributor.author	Rajamohan, R
dc.contributor.author	Bhattacharyya, J. C
dc.contributor.author	Subramanian, V
dc.contributor.author	Kuppuswamy, K
dc.date.accessioned	2006-04-11T08:24:35Z
dc.date.available	2006-04-11T08:24:35Z
dc.date.issued	1988-12
dc.identifier.citation	BASI, Vol. 16, No. 4, pp. 139-144	en
dc.identifier.uri	http://hdl.handle.net/2248/945
dc.description.abstract	Schmidt 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.extent	413983 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of Indian	en
dc.subject	Open cluster	en
dc.subject	Variable stars	en
dc.title	Variable stars in the old galactic cluster M67	en
dc.type	Article	en