Table 3
List of the selected stars.
| Spectral type | L | T eff | M |
| [L⊙] | [K] | [M⊙] | |
|
|
|||
| K (MS) | 0.35 | 4500 | 0.7 |
| G (MS) | 1 | 6000 | 1.0 |
| F (MS) | 7.5 | 6900 | 1.8 |
| A (MS) | 20 | 8500 | 2.4 |
|
|
|||
| T Tauri (PMS) | 0.95 | 4000 | 0.5 |
| Herbig Ae (PMS) | 43 | 9500 | 2.5 |
Notes. The denotation and the effective temperature of the main-sequence stars as spectral types refers to the Harvard Classification of Stars. We use the mass-luminosity relationship to estimate the stellar mass. (MS) = main-sequence stars; (PMS) = pre-main-sequence stars.
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