Table 1.
Simulations.
| Model | Star | β | e | rp | ra | va | rcirc | rcirc/rt |
|---|---|---|---|---|---|---|---|---|
| [R⊙] | [R⊙] | [m s−1] | [R⊙] | |||||
| S1.6 | S | 1 | 0.60 | 377.4 | 1509.6 | 1.5 ⋅ 107 | 607.5 | 1.6 |
| S1.7 | S | 1 | 0.70 | 377.4 | 2138.6 | 1.1 ⋅ 107 | 646.5 | 1.7 |
| S1.8 | S | 1 | 0.80 | 377.4 | 3396.5 | 7.1 ⋅ 106 | 685.7 | 1.8 |
| S1.9 | S | 1 | 0.90 | 377.4 | 7170.5 | 3.5 ⋅ 106 | 725.1 | 1.9 |
| S1.95 | S | 1 | 0.95 | 377.4 | 14718.3 | 1.7 ⋅ 106 | 744.9 | 2.0 |
| S1.99 | S | 1 | 0.99 | 377.4 | 75101.0 | 3.4 ⋅ 105 | 760.8 | 2.0 |
| S2.5 | S | 2 | 0.50 | 188.7 | 566.1 | 2.8 ⋅ 107 | 285.9 | 0.8 |
| S2.6 | S | 2 | 0.60 | 188.7 | 754.8 | 2.1 ⋅ 107 | 306.0 | 0.8 |
| S2.7 | S | 2 | 0.70 | 188.7 | 1069.3 | 1.6 ⋅ 107 | 326.3 | 0.9 |
| S2.8 | S | 2 | 0.80 | 188.7 | 1698.3 | 1.0 ⋅ 107 | 346.7 | 0.9 |
| S2.9 | S | 2 | 0.90 | 188.7 | 3585.2 | 5.0 ⋅ 106 | 367.4 | 1.0 |
| S2.95 | S | 2 | 0.95 | 188.7 | 7359.1 | 2.5 ⋅ 106 | 377.9 | 1.0 |
| S3.6 | S | 3 | 0.60 | 125.8 | 503.2 | 2.7 ⋅ 107 | 205.9 | 0.6 |
| S3.7 | S | 3 | 0.70 | 125.8 | 712.9 | 2.0 ⋅ 107 | 220.0 | 0.6 |
| S3.8 | S | 3 | 0.80 | 125.8 | 1132.2 | 1.3 ⋅ 107 | 234.4 | 0.6 |
| S3.9 | S | 3 | 0.90 | 125.8 | 2390.2 | 6.3 ⋅ 106 | 248.9 | 0.7 |
| S3.95 | S | 3 | 0.95 | 125.8 | 4906.1 | 3.1 ⋅ 106 | 256.3 | 0.7 |
| S4.7 | S | 4 | 0.70 | 94.3 | 534.6 | 2.3 ⋅ 107 | 167.4 | 0.4 |
| S4.8 | S | 4 | 0.80 | 94.3 | 849.1 | 1.5 ⋅ 107 | 178.8 | 0.5 |
| S4.9 | S | 4 | 0.90 | 94.3 | 1792.6 | 7.5 ⋅ 106 | 190.4 | 0.5 |
| S4.95 | S | 4 | 0.95 | 94.3 | 3679.6 | 3.7⋅106 | 196.3 | 0.5 |
| S5.7 | S | 5 | 0.70 | 75.5 | 427.7 | 2.6 ⋅ 107 | 136.4 | 0.4 |
| S5.8 | S | 5 | 0.80 | 75.5 | 679.3 | 1.7 ⋅ 107 | 146.1 | 0.4 |
| S5.9 | S | 5 | 0.90 | 75.5 | 1434.1 | 8.6 ⋅ 106 | 156.1 | 0.4 |
| S5.95 | S | 5 | 0.95 | 75.5 | 2943.7 | 4.3 ⋅ 106 | 161.2 | 0.4 |
| s1.6 | s | 1 | 0.60 | 162.6 | 650.5 | 2.3 ⋅ 107 | 264.4 | 1.6 |
| s1.7 | s | 1 | 0.70 | 162.6 | 921.5 | 1.7 ⋅ 107 | 282.1 | 1.7 |
| s1.8 | s | 1 | 0.80 | 162.6 | 1463.5 | 1.1 ⋅ 107 | 300.0 | 1.9 |
| s1.9 | s | 1 | 0.90 | 162.6 | 3089.7 | 5.4 ⋅ 106 | 318.2 | 2.0 |
| s1.95 | s | 1 | 0.95 | 162.6 | 6341.9 | 2.7 ⋅ 106 | 327.3 | 2.0 |
| s1.99 | s | 1 | 0.99 | 162.6 | 32360.1 | 5.3 ⋅ 105 | 334.7 | 2.0 |
| s2.5 | s | 2 | 0.5 | 81.3 | 243.9 | 4.3 ⋅ 107 | 126.2 | 0.8 |
| s2.6 | s | 2 | 0.60 | 81.3 | 325.2 | 3.4 ⋅ 107 | 135.9 | 0.8 |
| s2.7 | s | 2 | 0.70 | 81.3 | 460.7 | 2.5 ⋅ 107 | 145.9 | 0.9 |
| s2.8 | s | 2 | 0.80 | 81.3 | 731.8 | 1.7 ⋅ 107 | 156.1 | 1.0 |
| s2.9 | s | 2 | 0.90 | 81.3 | 1544.8 | 8.2 ⋅ 106 | 166.6 | 1.0 |
| s2.95 | s | 2 | 0.95 | 81.3 | 3171.0 | 4.1 ⋅ 106 | 171.9 | 1.0 |
Notes. For each model, the respective penetration factor β, eccentricity e, the pericentre distance rp, the apocentre distance ra, the velocity at apocentre va, the circularisation radius rcirc, and the ratio between rcirc and rt are reported. The model name includes the type of star, the penetration factor, and a number related to the eccentricity. A star with 10 M⊙, 5 R⊙ is dubbed as S (S star-like), while a star with 1 M⊙, 1 R⊙ is dubbed as s (solar-like). For instance, S1.6 is a model with an S star, β = 1, and e = 0.6.
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