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Table A.2

Stellar parameters of the single-lined members of RW clusters derived in the present work with the code ROTFIT.

Star Teff (K) log ɡ (dex) [Fe/H] (dex) SpT v sin i (km s−1) RV (km s−1) Prota$P_{{\rm{rot}}}^a$ (d) Memb?
Mel20-A1 5752 ± 69 4.35 ± 0.12 0.19 ± 0.07 G2.5V 1.9 ± 1.4 −5.98 ± 0.07 N
Mel20-A2 5843 ± 71 4.44 ± 0.11 −0.03 ± 0.10 G1V 11.6 ± 0.4 −1.62 ± 0.12 4.08 Y
Mel20-A3 6101 ± 70 4.20 ± 0.10 0.09 ± 0.08 F8V 4.4 ± 0.8 −0.68 ± 0.06 2.64 Y
Mel20-S1 5774 ± 71 4.37 ± 0.12 0.06 ± 0.08 G2V 8.2 ± 0.5 1.71 ± 0.08 3.98 Y
Mel20-S2 5781 ± 74 4.41 ± 0.12 0.10 ± 0.09 G2V 11.9 ± 0.3 0.41 ± 0.18 3.26 Y
Mel20-S3 5888 ± 110 4.44 ± 0.11 −0.03 ± 0.10 G1V 14.2 ± 0.3 −4.34 ± 0.16 3.90 Y?
Mel20-S8 5828 ± 72 4.44 ± 0.11 −0.02 ± 0.10 G2V 13.5 ± 0.5 −0.88 ± 0.15 3.05 Y
Plei-S3 6601 ± 119 4.14 ± 0.15 −0.00 ± 0.07 F6V 34.4±1.2 5.96 ± 0.59 6.16b Y
Plei-S5 5752 ± 67 4.39 ± 0.12 0.18 ± 0.08 G2V 9.3 ± 0.3 5.54 ± 0.12 6.84b Y
Plei-S7* 7800 ± 170 3.90 ± 0.20 −0.20 ± 0.11 A7III 18.4 ± 6.8 4.99 ± 0.23 Y
Plei-S8* 7900 ± 160 3.90 ± 0.20 −0.16 ± 0.11 A7III 31.8 ± 6.2 4.31 ± 0.43 N
Plei-S9* 8200 ± 100 4.10 ± 0.20 −0.20 ± 0.15 A4IV 40.7 ± 6.2 4.35 ± 1.02 Y
ASCC16-S1 5271 ± 89 4.53 ± 0.13 −0.00 ± 0.08 K0V 17.9 ± 0.4 21.27 ± 0.37 4.15 Y
ASCC16-S2 5184 ± 84 4.54 ± 0.10 −0.03 ± 0.08 K0V 18.3 ± 0.4 20.57 ± 0.34 4.06 Y
ASCC16-S6 5947±114 4.34 ± 0.13 0.07 ± 0.08 G2V 32.5 ± 0.4 21.37 ± 0.43 2.34 Y
ASCC16-S12 6233 ± 107 3.87 ± 0.14 −0.02 ± 0.09 F8IV 32.8 ± 0.6 20.58 ± 0.48 2.82 Y
ASCC19-S1 6724 ± 135 4.14 ± 0.14 −0.02 ± 0.08 F4V 53.5 ± 1.4 22.53 ± 0.52 3.77 Y
ASCC19-S2 6549 ± 170 4.09 ± 0.16 −0.06 ± 0.12 F5V 171.3 ± 7.2 25.16 ± 3.62 0.642 Y
ASCC19-S3 6657±119 4.14 ± 0.15 −0.01 ± 0.08 F4V 110.8 ± 4.4 21.16 ± 1.62 Y
ASCC19-S4 6062±119 4.15 ± 0.14 −0.03 ± 0.12 F9IV-V 13.8 ± 0.6 21.76 ± 0.28 4.26 Y
ASCC19-S5 6084 ± 73 4.20 ± 0.10 0.07 ± 0.10 F9IV-V 18.2±1.0 23.89 ± 0.32 3.42 Y
ASCC19-S6 5895 ± 96 4.35 ± 0.14 0.11 ± 0.09 G0V 45.5 ± 1.1 22.71 ± 1.20 2.09 Y
ASCC19-S14 6513 ±96 3.96 ± 0.12 −0.03 ± 0.09 F4V 17.0 ± 0.7 23.28 ± 0.18 0.665 Y
ASCC19-S15 6988 ± 121 4.13 ± 0.12 −0.04 ± 0.08 F1V 62.6 ± 1.9 22.70 ± 1.01 0.622 Y
ASCC19-S16 6750 ± 220 4.21 ± 0.13 −0.35 ± 0.15 F2V 64.8 ± 4.4 21.29 ± 0.84 Y
ASCC19-S17* 16 800 ± 900 4.00 ± 0.15 0.00 B4V 250.0 ± 10.0 22.06 ± 2.10 Y
ASCC19-S18* 14700 ± 600 4.10 ± 0.10 0.00 B6V 38.0 ± 5.0 21.48 ± 0.70 Y
ASCC19-S19* 14 600 ± 800 4.00 ± 0.20 0.00 B6V 190.0 ± 10.0 18.85 ± 1.85 Y
ASCC19-S20* 12 800 ± 300 4.00 ± 0.15 0.00 B8V 120.0 ± 13.2 23.60 ± 0.75 Y
ASCC19-S21* 9300 ±110 4.10 ± 0.15 0.00 A1V 36.9 ± 2.9 20.81 ± 0.27 Y
ASCC19-S22* 9400 ± 190 4.10 ± 0.20 0.00 A1V 49.5 ± 2.9 22.35 ± 0.46 Y
ASCC19-S23* 9200 ± 360 4.20 ± 0.25 0.00 A1V 137.4 ± 15.7 23.08 ± 1.34 Y
NGC2232-A2 5778 ± 73 4.39 ± 0.12 0.10 ± 0.09 G2V 17.9 ± 0.7 26.12 ± 0.26 2.79 Y
NGC2232-A3 5803 ± 69 4.40 ± 0.12 0.05 ± 0.07 G2V 13.1 ± 0.8 26.73 ± 0.24 3.97 Y
NGC2232-S3 5895 ± 111 4.45 ± 0.10 −0.04 ± 0.10 G1V 17.5 ± 0.4 26.05 ± 0.35 3.11 Y
NGC2232-S9 5849 ± 70 4.44 ± 0.11 −0.04 ± 0.10 G1V 17.6 ± 0.4 25.96 ± 0.32 2.61 Y
NGC2232-S11 6099 ± 75 4.17 ± 0.12 0.06 ± 0.09 F8V 12.1 ± 0.7 26.94 ± 0.14 3.06 Y
Ros6-S1 5942 ± 133 4.45 ± 0.10 −0.03 ± 0.10 G1V 13.7 ± 0.4 −8.13 ± 0.21 3.13 Y
Ros6-S2 6082 ± 71 4.30 ± 0.14 0.05 ± 0.09 G1V 17.3 ± 0.5 −8.20 ± 0.28 2.78 Y
Ros6-S5 5844 ± 68 4.43 ± 0.11 −0.03 ± 0.10 G1V 14.1 ± 0.3 −7.47 ± 0.22 3.24 Y
Ros6-S9 6088 ± 72 4.20 ± 0.10 0.07 ± 0.09 F8V 13.6 ± 0.4 −8.24 ± 0.12 3.27 Y
NGC7058-S1* 9200 ± 200 4.10 ± 0.10 0.00 A1 95.7 ± 2.6 −5.51 ± 2.02 Y?
NGC7058-S2* 9500 ± 200 4.30 ± 0.10 0.00 A0 42.3 ± 1.2 −8.05 ± 0.47 Y?
NGC7058-S3 6700 ± 148 4.15 ± 0.16 −0.02 ± 0.09 F5V 116.4 ± 5.4 −17.25 ± 3.18 Y
NGC7058-S4 6654 ± 122 4.14 ± 0.15 −0.01 ± 0.09 F3V 119.3 ± 4.3 −18.21 ± 2.85 Y
NGC7058-S5 6324 ± 147 4.10 ± 0.17 0.00 ± 0.08 F6IV 41.7 ± 2.2 −19.25 ± 1.01 1.48 Y
NGC7058-S6 6087 ± 72 4.21 ± 0.10 0.07 ± 0.10 F8V 24.7 ± 0.8 −-19.13 ± 0.40 13.65 Y
NGC7058-S7 5901 ± 120 4.44 ± 0.11 0.05 ± 0.07 G1V 14.8 ± 0.9 −19.03 ± 0.22 2.87 Y
NGC7058-S9 5785 ± 88 4.42 ± 0.12 −0.00 ± 0.10 G2V 6.6 ± 0.5 −33.25 ± 0.08 7.30 Y?
NGC7058-S10 5744 ± 83 4.38 ± 0.12 0.18 ± 0.08 G2V 4.0 ± 0.7 −19.41 ± 0.07 6.77 Y
NGC7058-S11 5682±114 4.45 ± 0.15 0.19 ± 0.10 G2.5V 5.8 ± 0.4 −19.43 ± 0.07 4.63 Y
NGC7058-S12 5491 ± 157 4.53 ± 0.11 0.11 ± 0.11 K0V 7.5 ± 0.5 −19.08 ± 0.09 4.82 Y
NGC7058-S13 5285 ± 90 4.55 ± 0.11 −0.00 ± 0.09 K0V 3.3 ± 0.8 −18.96 ± 0.06 5.69 Y

a Rotation periods derived in the present paper analysing the TESS light curves.

b Rotation periods derived by Rebull et al. (2016) with Kepler-K2.

* Warm stars. Atmospheric parameters derived with synthetic templates with solar metallicity as described in the text.

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