Abstract:
UBVRI photometry of the five open clusters Czernik 4, Berkeley 7, NGC 2236, NGC 7226 and King 12 has
been carried out using ARIES 104 cm telescope, Nainital. Fundamental cluster parameters such as fore-
ground reddening E (B-V), distance, and age have been derived by means of the observed two colour
and colour-magnitude diagrams, coupled to comparisons with theoretical models. E (B-V) values range
from 0.55 to 0.74 mag, while ages derived for these clusters range from ~10 to ~500 Myr. We have also
studied the spatial structure, mass function and mass segregation effects. The present study shows that
evaporation of low mass stars from the halo of the clusters increases as they evolve.
