Fig. 7
Location of ϵ Oct, β Peg, NU Pav, ψ Peg, and γ Hya in the HR diagram using our determination of the fundamental parameters. We also show the position of RS Cap by Martí-Vidal et al. (2011). The positions of the stars are compared with evolutionary tracks from Lagarde et al. (2012) for masses of 1.0 M⊙, 1.25 M⊙, 1.5 M⊙, 2.0 M⊙, 2.5 M⊙, 3.0 M⊙, 4.0 M⊙, and 6.0 M⊙.
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