Fig. 2
Dereddened color–magnitude diagram for the IC 1805 area. Dots are the cluster members according to Sanders (1972), crosses are field stars, some of them are possible cluster members. The gray line is ZAMS from Kazlauskas et al. (2006) for a distance modulus of V0 − MV = 11.5. The length of the reddening line corresponds to EB − V = 0.2.
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