Table 1.
Selection of parameters of the stellar models shown in Fig. 1.
| Model | M*/M⊙ | Zinit | R*/R⊙ | ρcen/g cm−3 | νdyn/μHz | Bcrit, cen/MG | Bcrit, H/MG | Varied parameter(s) |
|---|---|---|---|---|---|---|---|---|
| 1A | 1 | 0.02 | 1.8 | 9.1 ⋅ 103 | 42.6 | 86.2 | 36.9 | Bcen, ω, l |
| 1B | 1 | 0.02 | 2.7 | 5.1 ⋅ 104 | 22.0 | 25.0 | 2.5 | Bcen, ω |
| 1C | 1 | 0.02 | 12.3 | 2.2 ⋅ 105 | 2.3 | 0.29 | 0.006 | Bcen |
| 1a | 1 | 0.005 | 2.0 | 6.1 ⋅ 103 | 34.6 | 56.6 | 30.7 | Bcen |
| 1b | 1 | 0.005 | 3.2 | 6.1 ⋅ 104 | 17.1 | 14.8 | 1.4 | Bcen |
| 2A | 2 | 0.02 | 4.3 | 4.1 ⋅ 103 | 15.8 | 14.8 | 9.7 | Bcen, ω, l |
| 2B | 2 | 0.02 | 6.1 | 4.4 ⋅ 104 | 9.4 | 4.2 | 0.7 | Bcen, ω |
| 2C | 2 | 0.02 | 15.0 | 1.7 ⋅ 105 | 2.4 | 0.26 | 0.01 | Bcen |
| 2a | 2 | 0.005 | 4.5 | 1.0 ⋅ 104 | 15.0 | 12.2 | 6.0 | Bcen |
| 2b | 2 | 0.005 | 7.5 | 5.5 ⋅ 104 | 6.9 | 2.2 | 0.3 | Bcen |
Notes. The first column gives the name of the stellar model. The second column gives the stellar mass in solar masses, the third column the stellar metallicity, the fourth column the stellar radius in solar radii, and the fifth column the central density of the star. The sixth column shows the dynamic frequency νdyn, which is given by νdyn = ωdyn/(2π). The seventh and eighth columns show the critical magnetic field strengths in the center of the star (Bcrit, cen) and in the hydrogen-burning envelope (Bcrit, H) for dipole modes with ω = 10 ωdyn. The last column shows which parameters were varied during ray tracing analysis of a particular model. The values of models 2A, 2B, and 2C are similar to those of models A, B, and C of Loi (2020a), with the exception of Bcrit, cen of model 2A, which is smaller than the value of model A of Loi (2020a) by a factor of 2.
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