Table 3.
Best fits of the non-linear models.
Grid of models (Table 2) | Non-linear calculation | Fitting results | |||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
M⋆ | Teff (K) | L⋆ (L⊙) | R⋆ (R⊙) | P (days) | MKS (mag) | d (pc) | E(B − V) | α | β | λ0 (μm) |
![]() |
5850 | 4857 | 68.84 | 17.05 | −5.89 | 504.01.6 | 0.6640.006 | −0.270.03 | −1.790.32 | 1.820.14 | 6.45 | |
3 M⊙ | 5825 | 4785 | 69.52 | 17.17 | −5.90 | 504.91.3 | 0.6530.004 | −0.320.03 | −1.300.17 | 1.840.13 | 9.09 |
5800 | 4714 | 70.09 | 17.26 | −5.91 | 505.91.9 | 0.6430.007 | −0.370.05 | −1.060.23 | 1.830.23 | 25.86 | |
5825 | 6060 | 77.59 | 17.06 | −6.14 | 566.71.7 | 0.6550.004 | −0.290.02 | −1.550.20 | 1.790.12 | 4.16 | |
4 M⊙ | 5800 | 5961 | 78.37 | 17.13 | −6.15 | 567.21.7 | 0.6430.004 | −0.350.03 | −1.140.15 | 1.800.14 | 10.03 |
5775 | 5862 | 79.10 | 17.23 | −6.16 | 568.92.7 | 0.6310.008 | −0.430.07 | −0.870.24 | 1.770.28 | 33.72 | |
5800 | 7180 | 85.45 | 17.15 | −6.34 | 622.01.6 | 0.6450.003 | −0.320.02 | −1.340.12 | 1.760.09 | 2.50 | |
5 M⊙ | 5775 | 7061 | 86.25 | 17.21 | −6.35 | 622.62.0 | 0.6330.004 | −0.380.03 | −1.010.14 | 1.750.15 | 10.86 |
5750 | 6942 | 86.81 | 17.27 | −6.35 | 623.82.9 | 0.6220.008 | −0.460.08 | −0.800.22 | 1.720.27 | 29.76 | |
5775 | 8120 | 91.83 | 17.02 | −6.49 | 666.51.7 | 0.6360.002 | −0.340.01 | −1.190.08 | 1.720.07 | 1.98 | |
6 M⊙ | 5750 | 7994 | 92.61 | 17.09 | −6.50 | 667.62.1 | 0.6250.005 | −0.410.04 | −0.930.14 | 1.700.16 | 11.15 |
5725 | 7870 | 93.14 | 17.16 | −6.50 | 669.22.9 | 0.6150.008 | −0.480.08 | −0.760.21 | 1.650.26 | 25.59 | |
5750 | 9194 | 98.38 | 17.24 | −6.64 | 714.51.9 | 0.6300.002 | −0.350.01 | −1.160.08 | 1.670.07 | 1.79 | |
7 M⊙ | 5725 | 9031 | 99.07 | 17.28 | −6.64 | 715.02.2 | 0.6190.004 | −0.420.03 | −0.900.11 | 1.630.13 | 7.26 |
5700 | 8868 | 99.56 | 17.33 | −6.64 | 716.33.0 | 0.6080.007 | −0.490.07 | −0.730.18 | 1.560.24 | 18.78 | |
5750 | 10 069 | 102.14 | 16.97 | −6.73 | 748.43.7 | 0.6340.007 | −0.320.04 | −1.370.29 | 1.640.20 | 12.73 | |
8 M⊙ | 5725 | 9915 | 103.36 | 17.04 | −6.74 | 748.62.1 | 0.6200.002 | −0.380.01 | −1.020.06 | 1.610.06 | 1.91 |
5700 | 9764 | 104.02 | 17.11 | −6.74 | 750.42.6 | 0.6100.004 | −0.450.04 | −0.830.12 | 1.540.14 | 7.30 |
Notes. For each model computed (M⋆, Teff, L⋆), we derive the average stellar radius, R⋆ (R⊙), the pulsation period, P, in days, and the mean absolute magnitude in the KS-band, MKS. We simultaneously fit the distance, d (pc), color excess, E(B − V), and the parameters α, β, and λ0 of the CSE model (see Eq. (6)). The total is the mean reduced χ2 from the observations (see Sect. 4).
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