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Table 3

Previously known and calculated parameters of four CoRoT and Kepler δ Scuti stars.

Stars KIC 5892969 CID 546 CID 3619 CID 8669

Already Teff(K) 7560 ± 250 7600 ± 200 6990 ± 140 7000 ± 200
known log  geff 3.8 ± 0.3 3.9 ± 0.2 4.0 4.3 ± 0.2
parametersa vsini (km s-1) 10 17 108 200

Obtained Δν(μHz) 22.2 ± 0.4 55.4 ± 0.8 40.3 ± 0.6 55.0 ± 0.6
parameters s(μHz) 1.2 ± 0.1 7.1 ± 0.2 8.1 ± 0.5 16.9 ± 0.7

ρ(ρ) b 0.027 ± 0.001 0.169 ± 0.005 0.089 ± 0.005 0.17 ± 0.01
M(M) b 2.2 ± 0.3 1.5 ± 0.3 2.0 ± 0.1 2.4 ± 0.7
R(R) b 4.2 ± 0.5 2.09 ± 0.07 2.8 ± 0.1 2.4 ± 0.2
ϵ2(%)c 0.5 ± 0.1 3.0 ± 0.3 7.4 ± 0.9 17 ± 1
O(%)c 0.27 ± 0.03 1.5 ± 0.1 3.6 ± 0.4 8.0 ± 0.6
Calculated Rp(R) c 4.2 ± 0.5 2.07 ± 0.07 2.7 ± 0.1 2.3 ± 0.2
parameters Re(R) c 4.2 ± 0.5 2.10 ± 0.07 2.9 ± 0.1 2.5 ± 0.2
i(°) 15–35 88–90 55–90
Ω/Ωk(%) 14 ± 7 31 ± 3 48 ± 6 70 ± 7
log  Γ d 8.14 ± 0.08 8.15 ± 0.04 8.09 ± 0.01 8.11 ± 0.04
log  Ekin d 11.511 ± 0.004 12.77 ± 0.01 9.481 ± 0.003 11.57 ± 0.02
δTeff(%)c 0.13 ± 0.03 0.76 ± 0.08 0.61 ± 0.08 4.5 ± 0.3

Notes.

(a)

The parameters of KIC 5892969 are taken from Huber et al. (2014) and those of CoRoT stars are taken from the CorotSky Database (Charpinet et al. 2006).

(b)

Mean density (ρ), mass (M), and radius of a star with spherical symmetry (R; see Sect. 5).

(c)

Centrifugal to gravity force ratio (ϵ2), oblateness (O), polar and equatorial radii of the star (Rp and Re), and gravity-darkening effect (δTeff; see Sect. 2.2).

(d)

Convective efficiency and kinetic energy of the wave are both related to the convective layer of the star (see Sect. 2).

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