CCD Photometry of the Open Cluster BE 69

dc.contributor.author	Pandey, A. K
dc.contributor.author	Durgapal, A. K
dc.contributor.author	Bhatt, B. C
dc.contributor.author	Mohan, V
dc.contributor.author	Mahra, H. S
dc.date.accessioned	2008-07-22T11:50:16Z
dc.date.available	2008-07-22T11:50:16Z
dc.date.issued	1996
dc.identifier.citation	IAU Symposium, No. 174, pp. 339 - 340	en
dc.identifier.issn	0074-1809
dc.identifier.uri	http://hdl.handle.net/2248/2825
dc.description.abstract	The morphological features of CMDs of Be 69 are better understood in terms of convective overshooting.The Comparison of CMDs with the convective overshoot models (Bertelli et al. 1994)produces a good fit for metallicity Z=0.008, age=0.8, 1.0 billion yr and (m-M)=14.3, which corresponds to a distence of 2860 pc.	en
dc.format.extent	160578 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996IAUS..174..339P	en
dc.subject	CCD photometry	en
dc.subject	Open clusters	en
dc.title	CCD Photometry of the Open Cluster BE 69	en
dc.type	Article	en