Fig. 16.

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Proper-motion diagrams of stars in the field of view of NGC 1783 in five F438W magnitude intervals (left). The mF438W vs. mF438W − mF814W CMD for stars in the left panels is plotted on the middle. Stars within the black circles plotted in the proper-motion diagrams are considered probable cluster members and are colored black, whereas field stars are represented with aqua crosses. The right panel shows the mF438W vs. mF275W − mF438W CMD for probable cluster members, while the inset represents the Hess diagram of the CMD region around the upper MS.
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