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Table 1

Initial conditions of the ROLLIN’ simulations.

Name N 105 M 105 M ΔM/M r50% pc Σ 103 M pc−2 r50%/rj Vpeak km/s Vpeak0 β<50% log(trh/yr)
1.5M-A-R4-10 15 8.58 4 8.5 10 0.03 13.76 1.22 9.30
500k-A-R2-10 5 2.87 2 11.5 10 0.02 11.26 1.21 8.65
500k-A-R4-10 5 2.88 4 2.9 10 0.04 7.96 1.20 9.10
500k-A-R4-10-lC 5 2.88 4 2.9 10 0.04 7.96 1.20 9.10 level C sev
500k-C-R4-10 5 2.86 4 2.8 10 0.04 5.53 0.71 9.10
250k-A-R1-10 2.5 1.43 1 22.8 10 0.01 11.86 1.28 8.07
250k-A-R2-25 2.5 1.44 2 5.6 25 0.01 7.98 1.22 8.53
250k-A-R2-25-vlk 2.5 1.44 2 5.6 25 0.01 7.98 1.22 8.53 σnk = 5 km/s
250k-A-R2-10 2.5 1.44 2 5.6 10 0.03 7.98 1.22 8.53
250k-A-R2-5 2.5 1.44 2 5.6 5 0.05 8.31 1.27 8.53
250k-A-R4-25 2.5 1.44 4 1.5 25 0.02 5.63 1.22 8.97
250k-A-R4-25-imf50 2.5 1.37 4 1.4 25 0.02 5.50 1.22 8.98 mmax = 50 M
250k-A-R4-25-lk 2.5 1.44 4 1.5 25 0.02 5.63 1.22 8.97 σnk = 30 km/s
250k-A-R4-25-vlk 2.5 1.44 4 1.5 25 0.02 5.63 1.22 8.97 σnk = 5 km/s
250k-A-R4-25-retr 2.5 1.42 4 1.4 25 0.02 −5.61 −1.21 8.98 retrograde
250k-A-R4-10 2.5 1.44 4 1.5 10 0.05 5.63 1.22 8.97
250k-A-R4-10-retr 2.5 1.42 4 1.4 10 0.05 −5.61 −1.21 8.98 retrograde
250k-B-R4-25 2.5 1.41 4 1.4 25 0.02 4.92 0.99 8.98
250k-B-R4-25-lk 2.5 1.41 4 1.4 25 0.02 4.92 0.99 8.98 σnk = 30 km/s
250k-C-R2-10 2.5 1.43 2 5.6 10 0.03 5.52 0.70 8.53
250k-C-R4-25 2.5 1.43 4 1.4 25 0.02 3.90 0.71 8.97
250k-C-R4-25-lk 2.5 1.43 4 1.4 25 0.02 3.90 0.71 8.97 σnk = 30 km/s
250k-C-R4-10 2.5 1.43 4 1.4 10 0.05 3.90 0.71 8.97
250k-W6-R4-25 2.5 1.42 4 1.4 25 0.02 2.36 0.44 8.98
250k-W6-R4-25-retr 2.5 1.43 4 1.4 25 0.02 −2.31 −0.42 8.98 retrograde

Notes. Initial conditions of our set of simulations: the name of the simulation (see naming convention in Sect. 2), the number of stars N, the total mass M, the half-mass radius r50%, the mass surface density within the half-mass radius Σ, the distance d to the central point-mass galaxy, the filling factor defined as the ratio between the half-mass radius and the Jacobi radius rj, the peak of the rotation profile Vpeak, the Vpeak0 ratio with σ0 the central velocity dispersion, and the log of the half-mass radius relaxation time trh. The last column indicates additional information on the simulations (as described in Sect. 2), in particular nonstandard values of natal kicks σnk, level C stellar evolution, maximum value of the stellar mass function mmax and retrograde rotation.

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