Table A.2
Summary of strong correlations found for the stars analysed in cluster NGC6705.
| Star | ρw(RV,BIS) | ρw(RV,FWHM) | ρw (RV,Teff ) | ρw(RV,Hα1.6Å) | ρw(RV,Hα0.6Å) | A(Li) [dex] | Mass (M⊙) | υ sin(i) (km/s) | n |
|---|---|---|---|---|---|---|---|---|---|
| NGC6705No1090 | 1.380 | 3.800 | 6.050 | 9 | |||||
| NGC6705No1101 | ★ | 1.527 | 3.674 | 11.240 | 25 | ||||
| NGC6705No1111 | × | × | 1.425 | 3.618 | 7.110 | 10 | |||
| NGC6705No1117 | × | × | 1.567 | 3.521 | 9.440 | 10 | |||
| NGC6705No1145 | × | × | 1.385 | 3.355 | 7.300 | 11 | |||
| NGC6705No1184 | × | × | 0.215 | 3.448 | 4.420 | 11 | |||
| NGC6705No1248 | × | × | 1.525 | 3.455 | 8.430 | 9 | |||
| NGC6705No1256 | × | 1.591 | 3.146 | 4.470 | 14 | ||||
| NGC6705No1286 | × | × | 1.400 | 3.709 | 9.940 | 21 | |||
| NGC6705No1364 | 1.530 | 3.670 | 12.240 | 13 | |||||
| NGC6705No136 | × | × | 1.082 | 3.792 | 3.730 | 7 | |||
| NGC6705No1423 | 1.455 | 3.852 | 5.480 | 13 | |||||
| NGC6705No1446 | × | × | × | 1.194 | 3.451 | 7.140 | 6 | ||
| NGC6705No160 | 1.477 | 3.740 | 6.950 | 22 | |||||
| NGC6705No1625 | × | × | 1.088 | 3.087 | 4.100 | 19 | |||
| NGC6705No1658 | 1.512 | 3.910 | 7.290 | 28 | |||||
| NGC6705No1837 | × | × | × | 1.495 | 3.493 | 10.520 | 9 | ||
| NGC6705No2000 | × | 1.443 | 4.040 | 4.760 | 12 | ||||
| NGC6705No320 | × | × | × | 1.492 | 3.876 | 5.500 | 8 | ||
| NGC6705No411 | × | × | × | 1.573 | 3.193 | 6.470 | 8 | ||
| NGC6705No660 | × | × | × | 1.533 | 3.577 | 5.740 | 7 | ||
| NGC6705No669 | × | 1.511 | 3.451 | 8.930 | 6 | ||||
| NGC6705No686 | 1.467 | 3.727 | 9.480 | 6 | |||||
| NGC6705No779 | 1.569 | 3.397 | 5.570 | 22 | |||||
| NGC6705No816 | × | × | 1.533 | 3.956 | 8.770 | 6 | |||
| NGC6705No827 | × | -0.087 | 4.040 | 4.800 | 8 | ||||
| NGC6705No916 | × | 1.532 | 3.745 | 9.700 | 9 | ||||
| NGC6705No963 | 1.542 | 3.757 | 6.710 | 9 |
Notes. Each cross represents a correlation with BIS, FWHM, Teff or Hα > 0.4. Highlighted in blue are every star in this part of the sample that can be considered Li-rich, and highlighted in purple are all stars with considerable rotation, that is, υ sin(i) > 5 km/s. ★ indicates that a significant peak was found for the GLSP of the respective quantity which also appeared in RV. Also in this table are the values of the mass for each star (M) as well as the number of points (n) used to calculate the correlations.
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