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Fig. 5
Δν vs. νmax correlations (left) and H-R diagrams (right) obtained from BaSTI evolution models with 1.3 M⊙ and variable metallicity (top) and with [Fe/H] = 0.06 dex and variable mass (bottom). Note that in for the Δν vs. νmax correlations only stars with Teff < 5250 K have been taken into account.
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