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Fig. 3

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The location of the investigated CP stars in a log L/L versus log Teff diagram. Filled symbols denote members, whereas open symbols are non-members. The dashed line denotes the terminal-age main-sequence; the evolutionary tracks for individual masses are interpolated within the solar metallicity ones listed by Schaller et al. (1992), Schaerer et al. (1993a), Schaerer et al. (1993b), and Charbonnel et al. (1993).

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