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Table 1
Width of the BL for M∗ = 1.0 M⊙ and different stellar rotation rates ω = Ω∗/ΩK(R∗).
| ω | Δr [R∗] |  [cm s-1] |
|
|
|
|||
| 0.0 | 0.0074 | 493 × 106 | 1.013 |
| 0.2 | 0.0072 | 493 × 106 | 1.012 |
| 0.4 | 0.0074 | 492 × 106 | 1.012 |
| 0.6 | 0.0079 | 492 × 106 | 1.011 |
| 0.8 | 0.0104 | 490 × 106 | 1.008 |
Notes. By definition, the BL ranges from the surface of the star to the point where ∂Ω(r)/∂r = 0, i.e. where it has a maximum. Additionally, the absolute value of uϕ = Ω·r at rmax is given as .
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