Table 2
Stellar bins of the mock GC.
| ID | L(L⊙) | M(M⊙) | Teff (K) | log10 (g) (dex) | R (R⊙) | Weight | Vmic (km s−1) | Stage |
|---|---|---|---|---|---|---|---|---|
| 1 | 0.01 | 0.26 | 3928 | 5.03 | 0.26 | 7.408E+05 | 0.50 | MS |
| 2 | 0.11 | 0.53 | 4728 | 4.76 | 0.50 | 6.109E+04 | 0.50 | MS |
| 3 | 0.29 | 0.62 | 5460 | 4.66 | 0.61 | 1.906E+04 | 0.50 | MS |
| 4 | 0.52 | 0.67 | 5853 | 4.58 | 0.70 | 1.057E+04 | 0.50 | MS |
| 5 | 0.79 | 0.70 | 6126 | 4.49 | 0.79 | 7.031E+03 | 1.00 | MS |
| 6 | 1.14 | 0.73 | 6333 | 4.40 | 0.89 | 4.341E+03 | 1.00 | MS |
| 7 | 1.59 | 0.75 | 6474 | 4.31 | 1.00 | 3.321E+03 | 1.00 | MS |
| 8 | 2.15 | 0.76 | 6545 | 4.21 | 1.14 | 2.355E+03 | 1.00 | MS |
| 9 | 2.99 | 0.77 | 6480 | 4.05 | 1.37 | 1.755E+03 | 1.00 | TO/SGB |
| 10 | 4.65 | 0.78 | 5800 | 3.67 | 2.14 | 1.153E+03 | 1.11 | SGB |
| 11 | 10.3 | 0.79 | 5402 | 3.20 | 3.68 | 5.584E+02 | 1.26 | RGB |
| 12 | 23.5 | 0.79 | 5269 | 2.80 | 5.83 | 2.552E+02 | 1.40 | RGB |
| 13 | 48.2 | 0.79 | 5141 | 2.45 | 8.76 | 1.198E+02 | 1.52 | RGB |
| 14 | 88.2 | 0.79 | 5013 | 2.15 | 12.5 | 6.980E+01 | 1.62 | RGB |
| 15 | 139 | 0.79 | 4917 | 1.91 | 16.3 | 4.771E+01 | 1.69 | RGB |
| 16 | 225 | 0.79 | 4798 | 1.66 | 21.8 | 2.655E+01 | 1.78 | RGB |
| 17 | 370 | 0.79 | 4674 | 1.40 | 29.4 | 1.903E+01 | 1.87 | RGB |
| 18 | 623 | 0.79 | 4529 | 1.12 | 40.6 | 1.362E+01 | 1.96 | RGB |
| 19 | 1016 | 0.79 | 4382 | 0.85 | 55.4 | 8.028E+00 | 2.00 | RGB |
| 20 | 1554 | 0.79 | 4251 | 0.61 | 72.8 | 5.410E+00 | 2.00 | RGB |
| 21 | 47.5 | 0.60 | 9122 | 3.33 | 2.76 | 2.827E+01 | 1.80 | HB |
| 22 | 48.3 | 0.60 | 7563 | 3.00 | 4.05 | 2.827E+01 | 1.80 | HB |
Notes. L is the luminosity (given in solar units), M the mass of a star, Teff is the effective temperature, g the surface gravity, R the radius. The weight represents the total number of stars in this bin. Vmic is the micro-turbulent velocity in km −1s. The last column indicates the evolutionary stage of each bin: the main-sequence (MS), turn-off (TO), sub-giant (SGB), red giant branch (RGB), and the horizontal branch (HB). All models have the metallicity of [Fe/H] = − 2 dex.
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