Table 1
Parameters of the MARCS models used for the analysis of each RSG.
| RSG | log L/L⊙ | Teff (K) | log g | [Z] | ξ (km s−1) | M/M⊙ | R*/R⊙ |
|---|---|---|---|---|---|---|---|
| HD 95687 | 4.8 | 3500 | 0.0 | 0 | 5 | 15 | 690 |
| V602 Car | 5.1 | 3400 | −0.5 | 0 | 5 | 20 | 1015 |
Notes. From left to right: Luminosity log L/L⊙, effective temperature Teff, surface gravity log g, metallicity [Z], microturbulence ξ, and mass as in Arroyo-Torres et al. (2015). The last column shows the radius of the star in the photosphere in solar units (defined at τRoss = 2/3).
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