Table 1.
Summary of the main results for ESTER 2D models of a 15 M⊙ star with Z = 0.02 at ZAMS.
| ω | Ωeq/Ωc | log Ṁ | log TL |
|---|---|---|---|
| 0 | 0 | −8.40 | – |
| 0.1 | 0.105 | −8.41 | 8.60 |
| 0.2 | 0.210 | −8.42 | 8.61 |
| 0.3 | 0.313 | −8.43 | 8.62 |
| 0.4 | 0.415 | −8.44 | 8.63 |
| 0.5 | 0.516 | −8.46 | 8.64 |
| 0.6 | 0.615 | −8.47 | 8.65 |
| 0.7 | 0.714 | −8.48 | 8.65 |
| 0.8 | 0.812 | −8.49 | 8.64 |
| 0.9 (a) | 0.909 | −8.27 | 8.35 |
| 0.95 (a) | 0.957 | −8.25 | 8.22 |
| 0.99 (a) | 0.995 | −8.19 | 8.13 |
Notes. The first column reports the ratio of equatorial angular velocity to Keplerian angular velocity ω, the second column reports the critical angular velocity ratio Ωeq/Ωc, the third column is the global mass-loss rate log Ṁ, and the last column gives the ratio between total angular momentum and angular momentum loss rate 
. Ṁ is in M⊙ yr−1 and Tℒ in yr.
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