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Table A.1

Subset of collisions from our simulations.

m1 1 [M] R1 2 [R] m2 3 [M] R2 4 [R] d5 [AU] v6 [km s−1] b7 [AU] rp 8 [R1+R2] Δtcoll 9 [yr] Ek/Eb 10 Type11
2860.31 90.56 737.98 41.84 585.60 78.62 16.73 0.44 20.27 0.15 Binary
543.19 35.13 216.10 20.77 135.37 130.50 4.12 0.83 3.62 0.23 Hyperbolic
276.21 23.89 205.61 20.19 501.44 46.73 7.36 0.67 35.49 0.47 Hyperbolic
188.96 19.24 179.47 18.69 563.93 84.14 2.52 0.39 27.42 0.62 Hyperbolic
173.98 18.36 11.89 3.98 720.51 32.58 0.44 0.01 80.72 0.04 Hyperbolic
169.79 18.11 78.02 11.62 1346.44 52.02 1.20 0.06 108.87 0.27 Hyperbolic
148.23 16.76 29.64 6.70 2371.13 126.80 0.83 0.32 86.93 0.11 Hyperbolic
79.46 11.75 10.94 3.79 1167.97 19.98 4.06 0.57 220.12 0.08 Hyperbolic
37.50 7.65 7.68 3.10 1110.80 27.30 0.32 0.02 173.65 0.11 Hyperbolic
18.60 5.13 1.88 1.39 800.18 16.16 1.66 0.66 201.31 0.05 Hyperbolic

Notes. (1) Mass of the most massive star. (2)Radius of the most massive star. (3)Mass of the least massive star. (4)Radius of the least massive star. (5)Distance between the stars. (6)Magnitude of the relative velocity between the stars. (7)Impact parameter. (8) pericenter distance in units of the sum of the radii of the stars. (9)Time until the collision of the stars, as obtained from the simulation. (10) Kinetic energy of the collision divided by the binding energy of the most massive star. (11) Type of orbit that led to the collision.

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