Table 9.
Dispersion (σX) and full amplitude range of the abundances (AX, i.e., difference between highest and lowest value) and mean of the quoted uncertainties for each cluster (left) and comparison with L16 results for the elements in common (right).
Cluster | Hyades |
NGC 2632 |
Ruprecht 147 |
Element | σXL16 | σXhere | ||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
σX | AX | Unc. | σX | AX | Unc. | σX | AX | Unc. | ||||
Na I | 0.025 | 0.151 | 0.021 | 0.052 | 0.245 | 0.024 | 0.070 | 0.268 | 0.035 | Na I | 0.021 | 0.017 |
Mg I | 0.026 | 0.126 | 0.026 | 0.048 | 0.172 | 0.013 | 0.047 | 0.166 | 0.019 | Mg I | 0.035 | 0.024 |
Al I | 0.033 | 0.149 | 0.029 | 0.057 | 0.214 | 0.021 | 0.067 | 0.264 | 0.038 | Al I | 0.046 | 0.029 |
Si I | 0.026 | 0.141 | 0.028 | 0.031 | 0.144 | 0.044 | 0.042 | 0.159 | 0.039 | Si I | 0.023 | 0.025 |
Ca I | 0.029 | 0.129 | 0.032 | 0.044 | 0.193 | 0.047 | 0.031 | 0.128 | 0.070 | Ca I | 0.023 | 0.023 |
Sc II | 0.032 | 0.141 | 0.034 | 0.047 | 0.195 | 0.041 | 0.065 | 0.355 | 0.046 | Ti I | 0.029 | 0.029 |
Ti I | 0.033 | 0.151 | 0.035 | 0.034 | 0.116 | 0.056 | 0.037 | 0.117 | 0.046 | Ti II | 0.032 | 0.028 |
Ti II | 0.029 | 0.135 | 0.035 | 0.044 | 0.190 | 0.057 | 0.043 | 0.175 | 0.043 | V I | 0.026 | 0.037 |
V I | 0.035 | 0.155 | 0.033 | 0.062 | 0.268 | 0.072 | 0.049 | 0.166 | 0.045 | Cr I | 0.026 | 0.021 |
Cr I | 0.026 | 0.121 | 0.038 | 0.045 | 0.207 | 0.058 | 0.053 | 0.192 | 0.076 | Mn I | 0.026 | 0.031 |
Mn I | 0.028 | 0.130 | 0.036 | 0.044 | 0.173 | 0.036 | 0.053 | 0.160 | 0.058 | Fe I | 0.023 | 0.024 |
Fe I | 0.026 | 0.108 | 0.035 | 0.040 | 0.162 | 0.050 | 0.043 | 0.192 | 0.062 | Co I | 0.030 | 0.024 |
Fe II | 0.028 | 0.125 | 0.035 | 0.045 | 0.170 | 0.039 | 0.061 | 0.309 | 0.046 | Ni I | 0.028 | 0.023 |
Co I | 0.029 | 0.140 | 0.027 | 0.059 | 0.213 | 0.043 | 0.055 | 0.246 | 0.051 | Cu I | 0.036 | 0.025 |
Ni I | 0.027 | 0.128 | 0.031 | 0.039 | 0.147 | 0.051 | 0.056 | 0.254 | 0.068 | Ba II | 0.031 | 0.037 |
Cu I | 0.026 | 0.134 | 0.045 | 0.050 | 0.201 | 0.099 | 0.055 | 0.237 | 0.114 | |||
Y II | 0.040 | 0.180 | 0.042 | 0.065 | 0.245 | 0.069 | 0.115 | 0.557 | 0.056 | |||
Ba II | 0.038 | 0.179 | 0.044 | 0.079 | 0.305 | 0.033 | 0.089 | 0.417 | 0.056 | |||
La II | 0.042 | 0.154 | 0.098 | 0.031 | 0.074 | 0.049 | 0.037 | 0.092 | 0.044 | |||
Ce II | 0.044 | 0.129 | 0.145 | 0.021 | 0.051 | 0.087 | 0.017 | 0.042 | 0.162 | |||
Nd II | 0.050 | 0.229 | 0.061 | 0.097 | 0.394 | 0.086 | 0.083 | 0.287 | 0.075 | |||
Eu II | 0.020 | 0.049 | 0.110 | 0.022 | 0.049 | 0.095 | 0.025 | 0.063 | 0.179 |
Notes. The dispersions were obtained using the subsample of stars of L16 (σXhere) and their values (σXL16).
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