Fig. 1
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Reddening corrected color–magnitude diagram of NGC 3114. Black filled circles are kinematically main-sequence member stars from Tables 2 and 3 of González & Lapasset (2001). Our program stars are identified by red filled squares. We also show the isochrone of Bertelli et al. (1994) for log t = 8.2 (0.16 Gyr), Z = 0.02, and Y = 0.28.
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