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.
