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Table 1
Width of the boundary layer for a parameter variation of the stellar mass and the mass-accretion rate.
| M ∗ [M⊙] | Ṁ [M⊙/ yr] | Δr [R∗] | sim. time [orbits] |
|
|
|||
| 0.8 | 1 × 10-8 | 0.0100 | 688 |
| 0.8 | 1 × 10-9 | 0.0066 | 604 |
| 0.8 | 1 × 10-10 | 0.0048 | 395 |
| 1.0 | 1 × 10-8 | 0.0084 | 395 |
| 1.2 | 1 × 10-8 | 0.0064 | 387 |
Notes. By definition, the BL ranges from the surface of the star to the point where ∂Ω(r) /∂r = 0, that is, where it has a maximum.
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