Table 3.
Models with both simplified stellar evolution and SG stars.
| Initial |
Final |
|||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Model (a) | W0, FG | rh, FG | Segr | MSG | W0, SG | rh, SG | MFG | MSG |  (fenriched) |
 |
rh, FG | rh, SG | rh, tot | log(ρc) |
| (pc) | (105 M⊙) | (pc) | (105 M⊙) | (105 M⊙) | (pc) | (pc) | (pc) | (M⊙ pc−3) | ||||||
| 5N7M3.70 | 5 | 37 | N | 30 | 7 | 3.7 | 35.4 | 18.0 | 0.44 (0.34) | 0.16 | 25.0 | 12.5 | 19.9 | 3.61 |
| 5N7M3.710 | 5 | 37 | N | 30 | 7 | 3.7 | 33.6 | 18.5 | 0.49 (0.35) | 0.15 | 25.5 | 10.1 | 18.9 | 4.08 |
| 5N7M3.7K | 5 | 37 | N | 30 | 7 | 3.7 | 36.3 | 19.8 | 0.49 (0.35) | 0.14 | 24.1 | 9.34 | 17.3 | 4.11 |
| 5Y7M3.7K | 5 | 37 | Y | 30 | 7 | 3.7 | 26.3 | 19.3 | 0.58 (0.42) | 0.13 | 27.4 | 9.22 | 18.2 | 4.41 |
| 5Y7M1K | 5 | 37 | Y | 30 | 7 | 1 | 22.9 | 15.7 | 0.46 (0.40) | 0.16 | 27.8 | 22.4 | 25.4 | 2.36 |
| 5Y5M1K | 5 | 37 | Y | 30 | 5 | 1 | 21.0 | 15.5 | 0.48 (0.42) | 0.15 | 27.7 | 22.4 | 25.2 | 2.36 |
| 5Y7m1K | 5 | 37 | Y | 7 | 7 | 1 | 21.9 | 4.42 | 0.23 (0.16) | 0.03 | 32.1 | 20.2 | 29.9 | 2.15 |
| 2N7M1K | 2 | 60 | N | 30 | 7 | 1 | 12.6 | 14.1 | 0.58 (0.52) | 0.15 | 24.4 | 19.9 | 21.8 | 2.34 |
| 4N7M4.5K | 4 | 45 | N | 30 | 7 | 4.5 | 27.8 | 18.8 | 0.58 (0.40) | 0.13 | 29.3 | 7.84 | 19.4 | 4.90 |
| 2N7m6K | 2 | 60 | N | 7 | 7 | 6 | 3.02 | 3.33 | 0.56 (0.52) | 0.04 | 13.2 | 10.8 | 11.8 | 2.55 |
| 2N5m6K | 2 | 60 | N | 7 | 5 | 6 | 2.93 | 3.50 | 0.59 (0.54) | 0.03 | 12.9 | 10.2 | 11.3 | 2.45 |
| 2N7m1K | 2 | 60 | N | 7 | 7 | 1 | 1.89 | 2.00 | 0.59 (0.52) | 0.05 | 10.9 | 6.19 | 8.32 | 4.98 |
| 2N5m1K | 2 | 60 | N | 7 | 5 | 1 | 2.15 | 2.09 | 0.57 (0.49) | 0.05 | 10.7 | 6.11 | 8.25 | 4.47 |
Notes. The initial FG mass of each simulated cluster is M0 = 8.4 × 106 M⊙, after the removal of 16% of its mass.
Model name: W0, FG + Y or N = with or without segregation + W0, SG + m pr M = low or high initial MSG + initial rh, SG + σ0, SG (K = King velocity dispersion). Columns: 1) name of the model; 2) W0 of the FG; 3) half-mass radius of the FG; 4) primordial segregation of the FG (N = non-segregated, Y = segregated), 5) mass of the SG; 6) W0 of the SG; 7) half-mass radius of the SG; 8) total mass of FG bound stars; 9) total mass of SG bound stars; 10) fraction of SG stars within the half-mass radius of the whole cluster (fraction of SG stars of the whole cluster); 11) fraction of SG stars among unbound stars flostSG = MlostSG/Mlosttot, where MlostSG and 
are the mass of unbound SG and the total mass of unbound stars, respectively; 12) half-mass radius of the bound FG; 13) half-mass radius of the bound SG; 14) half-mass radius of the whole cluster (i.e., only bound stars); 15) central density.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.