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In this paper we study the evolution of the core and corona of nine open clusters using the projected radial density profiles derived from homogeneous CCD photometric data obtained with the 105 cm Kiso Schmidt telescope. The age and galactocentric distance of the target clusters vary from 16 to 2000 Myr and 9 to 10.8 kpc, respectively. Barring Be 62, which is a young open cluster, other clusters show a uniform reddening across the cluster region. The reddening in Be 62 varies from E(B À V ) min ¼ 0:70 mag to E(B À V ) max ¼ 1:00 mag. The coronae of six of the clusters in the present sample are found to be elongated; however, on the basis of the present sample it is not possible to establish any correlation between the age and shape of the core. The elongated core in the case of the young cluster Be 62 may reflect the initial conditions in the parental molecular cloud. The other results of the present study are as follows:(1) Core radius r c and corona size r cn /cluster radius r cl are linearly correlated.(2) The r c , r cn , and r cl are linearly correlated with the number of stars in that region. (3) In the age range 10Y1000 Myr, the core and corona shrink with age. (4) We find that in the galactocentric distance range 9Y10 kpc, the core and corona/cluster extent of the clusters increase with the galactocentric distance.

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