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Table 1
Parameters of the two dynamical models (adopted from Nowotny et al. 2010) used in this study.
| Model: | W | M |
|
|
||
| L⋆ [L⊙] | 7000 | 7000 |
| M⋆ [M⊙] | 1.0 | 1.5 |
| T⋆ [K] | 2800 | 2600 |
| R⋆ [R⊙] | 355 | 412 |
|
|
||
| [Fe/H] | 0 | 0 |
| C/O [by number] | 1.4 | 1.4 |
|
|
||
| Period [days] | 390 | 490 |
| Δup [km s-1] | 2 | 6 |
| f L | 1.0 | 1.5 |
Notes. While model W represents a pulsating star without mass loss, model M represents a Mira developing a wind. Note that the radius is calculated from luminosity and temperature.
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