Fig. 1
Large separation as a function of effective temperature of the stars used in this study. The error bars on the large separations are within the thickness of the symbol. The evolutionary tracks for stars of mass from 0.8 M⊙(most right) to 1.5 M⊙ (most left) (by step of 0.1 M⊙) are shown as dotted lines. The tracks are derived from Marigo et al. (2008).
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