Table 4
Parameters for the model stars SRV and MIRA used to calculate hydrodynamic trajectories.
| Model | n0 | T0 | v∞ | vs | pp |
|---|---|---|---|---|---|
| SRV | 1.e14 | 2400 | 5.7 | 10 | 332 |
| MIRA | 4.e14 | 2000 | 17.7 | 20 | 450 |
Notes. Number densities n0 ≡ n(1 R⋆) are given in units of cm−3, temperatures T0 ≡ T(1 R⋆) in units of K, the terminal velocity (v∞) and shock velocity (vs) in units of km s−1, and the pulsation period (pp) in units of days. Number densities and temperatures correspond to their values at the photosphere (1 R⋆).
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