UBVRI CCD photometric studies of open clusters Berkeley 15, Czernik 18 and NGC 2401

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/742

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DC Field	Value	Language
dc.contributor.author	Sujatha, S	-
dc.contributor.author	Babu, G. S. D	-
dc.contributor.author	Ananthamurthy, S	-
dc.date.accessioned	2006-03-13T11:03:19Z	-
dc.date.available	2006-03-13T11:03:19Z	-
dc.date.issued	2004-12	-
dc.identifier.citation	BASI, Vol. 32, No. 4, pp. 295-309	en
dc.identifier.uri	http://hdl.handle.net/2248 /742	-
dc.description.abstract	CCD photometric observations of three open clusters Berkeley 15 (=OCl 414), Czernik 18 (=OCl 426) and NGC 2401 (=OCl 588), obtained for the first time in UBVRI filters down to V=20 mag, are presented here. They are located at distances of 1259, 955 and 3467 parsecs with their respective ages estimated as ~5 x 109 years, ~0.8 to 1 x 109 years and ~1 x 109 years. While OCl 414 and OCl 426 are in the direction of the Auriga - Perseus constellations, OCl 588 is placed in the direction of Ophiuchus constellation in our Galaxy. The clusters studied here are of intermediate and old age category	en
dc.format.extent	112387 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Open clusters	en
dc.subject	distances	en
dc.subject	ages	en
dc.title	UBVRI CCD photometric studies of open clusters Berkeley 15, Czernik 18 and NGC 2401	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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