Table 1.
Parameters of stellar structure models produced with MESA for the hydrodynamic simulations.
| Age | R | L | Teff | P | |
|---|---|---|---|---|---|
| ceph5 | 8.25 | 2.95 | 1.73 | 5.71 | 4.74 |
| ceph6 | 7.83 | 3.95 | 2.40 | 5.36 | 7.64 |
| ceph7a | 4.96 | 5.00 | 3.30 | 5.16 | 10.39 |
| ceph7b | 5.37 | 5.54 | 4.14 | 5.19 | 12.41 |
| ceph8 | 3.33 | 7.38 | 5.15 | 4.75 | 19.00 |
| ceph9 | 2.95 | 8.46 | 9.00 | 5.10 | 22.00 |
Notes. The star’s age in 107 years, the radius of the photosphere of the star in 1012 cm, the luminosity L of the star at the photosphere in 103 L⊙, the effective temperature of the star Teff at the photosphere in 103 Kelvin, and the pulsation period P in days, determined with MESA-RSP are included. For each simulation the metallicity z is equal to 0.020 and the helium mass fraction y is set at 0.29.
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