Open Access

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.

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.