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Table 3
Description of the online tables containing the results of our evolutionary calculations as a function of time, for given initial composition, initial mass and initial rotation rate.
| Stellar | Surf. | Surface & core | ||
| parameters | abun | isotope mass fractions | ||
| Age (t [yrs]) | H | 1H | ||
| Mass (m [M⊙]) | He | 3He | 4He | |
| Eff. temp. (Teff[K]) | Li | 7Li | ||
| Luminosity (log (L/L⊙)) | Be | 9Be | ||
| Radius (R [R⊙]) | B | 10B | 11B | |
| Mass loss rate (Ṁ [M⊙/yr]) | C | 12C | 13C | |
| Surface gravity (log g) | N | 14N | 15N | |
| Surface velocity (3surf [km s-1]) | O | 16O | 17O | 18O |
| Rotation period (P [days]) | F | 19F | ||
| Critical velocity (3crit [km s-1]) | Ne | 20Ne | 21Ne | 22Ne |
| Eddington factor (Γe) | Na | 23Na | ||
| Mg | 24Mg | 25Mg | 26Mg | |
| Al | 26Al | 27Al | ||
| Si | 28Si | 29Si | 30Si | |
| Fe | 56Fe | |||
Notes. The critical velocity is computed as 
= GM/R(1 − Γe), where Γe denotes the Eddington factor due to electron scattering.
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