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Table 12.

Observed and theoretical periods of the asteroseismological solution for EC 20058 in the case 1, using 11 periods [M = 0.664 M, Teff = 26 380 K].

O Πk k m δΠk Unstable
(s) (s) (s) (10−13 s/s)
195.0 1 193.39 2 6 0 1.61 0.40 Yes
204.6 ? 204.19 1 3 0 0.41 0.44 Yes
207.6 2 206.45 2 7 0 1.15 0.47 Yes
256.852 2 248.42 2 9 0 8.43 0.60 Yes
274.7 1 275.87 1 5 0 −1.17 0.53 Yes
280.983 2 275.87 1 5 0 5.11 0.53 Yes
286.6 ? 293.03 2 11 0 −6.43 0.69 Yes
333.5 ? 332.28 2 13 0 1.22 0.750 Yes
350.6 2 352.48 2 14 0 −1.88 0.62 Yes
525.4 1 524.05 1 12 0 1.35 1.11 Yes
539.8 ? 538.01 2 23 0 1.79 1.24 Yes

Notes. Periods are in seconds and rates of period change (theoretical) are in units of 10−13 s/s. represents the period differences, the harmonic degree, k the radial order, m the azimuthal index. The last column gives information about the pulsational stability/instability nature of the modes.

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