Table 3
Parameters derived for stars of spectral class M.
| ID |  |
Teff,TiO (K) | AV (mag) | log g (dex) | Mbol (mag) | log(L*/L⊙) (dex) | R* (R⊙) |
|---|---|---|---|---|---|---|---|
| SMC3 | 1.0 |  |
 |
+0.3 ± 0.1 |  |
 |
 |
| LMC1 | 1.0 |  |
 |
+0.4 ± 0.1 |  |
 |
 |
| LMC2 | 5.2 |  |
 |
>+1.0 |  |
 |
 |
| LMC3 | 2.9 |  |
 |
+0.5 ± 0.1 |  |
 |
 |
| LMC4 | 1.1 |  |
 |
+0.1 ± 0.1 |  |
 |
 |
| LMC5 | 1.6 |  |
 |
+0.3 ± 0.1 |  |
 |
 |
| LMC6 | 1.9 |  |
 |
> +0.5 |  |
 |
 |
| LMC7 | 3.5 |  |
 |
> +0.5 |  |
 |
 |
| LMC8 | 2.5 |  |
 |
+0.5 ± 0.1 |  |
 |
 |
Notes. The errors presented for Teff,TiO and AV correspond to the edges of the 1σ contour. For LMC6 and LMC7, we give a lower limit on the surface gravity. By eye we noticed that +0.5 came close to fitting these stars, but the real surface gravity is likely in the range [+0.5,+1.0], which could not be fitted with the models we have available. For LMC2, it is evident that the surface gravity is higher than +1.0, and therefore too compact to be an RSG.
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