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Table 4.

Mean RV and metallicity for the observed clusters.

Cluster RV σRV [Fe/H] σ[Fe/H] N
(km s−1) (km s−1) (dex) (dex)
ASCC 11 −10.94 0.19 −0.14 0.05 1
Alessi 1 −4.37 0.85 0.00 0.08 4
Alessi-Teusch 11 −27.11 0.12 −0.19 0.05 1
Basel 11b 2.17 0.37 −0.01 0.05 3
COIN-Gaia 30 −26.66 0.13 0.03 0.05 1
Collinder 463 −10.66 0.98 −0.15 0.05 2
Gulliver 18 −1.97 0.18 −0.10 0.05 1
Gulliver 24 −30.37 0.16 −0.10 0.05 1
Gulliver 37 −4.59 (a) 0.17 0.10 0.05 1
NGC 2437 49.13 (a) 0.93 0.00 0.04 7
NGC 2509 61.63 0.14 −0.10 0.06 1
NGC 2548 8.41 (a) 0.46 −0.02 0.03 4
NGC 7082 −11.89 0.15 −0.15 0.05 1
NGC 7209 −18.49 0.51 −0.04 0.04 2
Tombaugh 5 −21.21 1.30 0.05 0.05 3
UPK 219 −0.07 0.15 0.02 0.05 1
Comparison clusters
Collinder 350 −15.14 1.16 0.00 0.05 1
NGC 2682 34.28 (a) 0;65 0.03 0.03 4

Notes.

(a)

Binary systems (see Table 2).

When only 1 star is observed, σ is the error, nor the dispersion.

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