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Table 5:

Global parameters for the four stars.
Star $\nu_{\rm max}$ $\Delta \nu$ HA/HB $T_{\rm eff}$ M R
  $\mu $Hz $\mu $Hz   K $M_{\odot}$ $R_{\odot}$
102732890 25.5 3.15 $1.1 \pm 0.1$ 4140 1.2 13.0
102788308 51.8 5.3 $1.6 \pm 0.1$ 4260 1.3 9.4
102762620 21.9 2.7 $0.3 \pm 0.03$ 4355 1.5 15.6
102767771 25.8 3.1 $0.4 \pm 0.1$ 4250 1.4 13.7

Notes. Frequency of maximum oscillation power ( $\nu_{\rm max}$) and the large frequency separation ($\Delta \nu$) in $\mu $Hz, the ratio of the mean height of ridge ``A'' to ridge ``B'' for which the degrees are unknown, the effective temperature ( $T_{\rm eff}$) in K and the asteroseismic mass and radius in $M_{\odot}$ and $R_{\odot}$, respectively. Errors are typically of the order of 1 and 0.05 $\mu $Hz for $\nu_{\rm max}$ and $\Delta \nu$, 100 K for $T_{\rm eff}$ and below 20 and 10 % for M and R, respectively.


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