Table A.1
Theoretical and observational quantities for 47 Tuc 1G isochrone
| M/M⊙ | Teff | log(L/L⊙) | mF322W2 | mF115W - mF322W2 | mF150W2 - mF322W2 | (Lpp/L)12Gyr | (Lpp/L)max |
|---|---|---|---|---|---|---|---|
| 0.060 | 858.0 | −5.56 | 14.70 | 1.90 | 1.95 | 0.0014 | 0.08 |
| 0.061 | 878.5 | −5.52 | 14.64 | 1.85 | 1.90 | 0.0019 | 0.10 |
| 0.062 | 899.0 | −5.48 | 14.54 | 1.82 | 1.82 | 0.0025 | 0.12 |
| 0.063 | 923.5 | −5.44 | 14.49 | 1.80 | 1.80 | 0.0032 | 0.14 |
| 0.064 | 947.0 | −5.39 | 14.41 | 1.75 | 1.72 | 0.0043 | 0.17 |
| 0.065 | 970.5 | −5.35 | 14.33 | 1.73 | 1.68 | 0.0057 | 0.21 |
| 0.066 | 996.5 | −5.31 | 14.23 | 1.70 | 1.63 | 0.008 | 0.25 |
| 0.067 | 1022.9 | −5.27 | 14.16 | 1.65 | 1.63 | 0.012 | 0.30 |
| 0.068 | 1047.7 | −5.22 | 14.06 | 1.62 | 1.63 | 0.019 | 0.36 |
| 0.069 | 1079.3 | −5.07 | 13.95 | 1.60 | 1.62 | 0.034 | 0.41 |
| 0.070 | 1206.4 | −4.97 | 13.54 | 1.91 | 1.61 | 0.047 | 0.50 |
| 0.071 | 1292.7 | −4.84 | 13.16 | 2.00 | 1.55 | 0.11 | 0.60 |
| 0.072 | 1359.2 | −4.73 | 12.77 | 2.31 | 1.50 | 0.31 | 0.70 |
| 0.073 | 1447.4 | −4.58 | 12.45 | 2.37 | 1.46 | 0.72 | 0.82 |
| 0.074 | 1580.9 | −4.39 | 12.09 | 1.95 | 1.25 | 0.95 | 0.97 |
| 0.075 | 1719.5 | −4.22 | 11.80 | 1.57 | 1.10 | 1.00 | 1.00 |
| 0.076 | 1828.5 | −4.096 | 11.55 | 1.41 | 0.95 | 1.00 | 1.00 |
| 0.077 | 1937.7 | −3.97 | 11.38 | 1.25 | 0.81 | 1.00 | 1.00 |
| 0.078 | 2024.9 | −3.88 | 11.20 | 1.15 | 0.75 | 1.00 | 1.00 |
| 0.079 | 2100.4 | −3.80 | 11.08 | 1.06 | 0.69 | 1.00 | 1.00 |
| 0.080 | 2172.2 | −3.73 | 10.94 | 1.08 | 0.66 | 1.00 | 1.00 |
| 0.085 | 2457.0 | −3.46 | 10.34 | 1.04 | 0.60 | 1.00 | 1.00 |
| 0.090 | 2648.5 | −3.28 | 9.92 | 1.07 | 0.59 | 1.00 | 1.00 |
| 0.100 | 2875.4 | −3.04 | 9.40 | 1.09 | 0.58 | 1.00 | 1.00 |
| 0.120 | 3069.0 | −2.79 | 8.82 | 1.10 | 0.57 | 1.00 | 1.00 |
| 0.150 | 3202.6 | −2.55 | 8.29 | 1.09 | 0.56 | 1.00 | 1.00 |
| 0.200 | 3321.2 | −2.28 | 7.67 | 1.07 | 0.54 | 1.00 | 1.00 |
| 0.250 | 3410.4 | −2.08 | 7.20 | 1.06 | 0.52 | 1.00 | 1.00 |
| 0.300 | 3485.8 | −1.91 | 6.82 | 1.06 | 0.51 | 1.00 | 1.00 |
| 0.400 | 3652.6 | −1.62 | 6.14 | 1.08 | 0.50 | 1.00 | 1.00 |
| 0.500 | 3931.0 | −1.28 | 5.36 | 1.10 | 0.49 | 1.00 | 1.00 |
Notes. The table lists various theoretical and observational properties of stellar models of different mass (reported in col. 1) with the chemical composition used to model the 1G of the cluster, namely [Fe/H] = −0.78, helium mass fraction Y = 0.255, and [O/Fe] = +0.4. Col. 2 and 3 give the effective temperature and luminosity, whereas col. from 4 to 6 report mF322W2 magnitude, the (mF115W - mF322W2) and (mF150W - mF322W2) colours, respectively. Col. 7 and 8 give the fractional p-p luminosity at the age of 12 Gyr and the largest p-p luminosity reached during the evolution.
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