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CCD Photometry of the Open Cluster BE 69
Published online by Cambridge University Press: 25 May 2016
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 a metallicity Z=0.008, age = 0.8 − 1.0 billion yr and (m-M) = 14.3, which corresponds to a distance of 2860 pc.
- Type
- Posters: Observations of Star Clusters
- Information
- Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996 , pp. 339 - 340
- Copyright
- Copyright © Kluwer 1996