Table 1: Mean radial velocities and general information for 37 members in Melotte 20.

He 
V B-V V-Ik U-B Sp.T. $\mu_{\alpha}$ $\mu_{\delta}$ Prob $V_{\rm r}$ $\epsilon$ n $\Delta T$ P($\chi^2$) $Vr_{{\rm litt}}$ N Astr Diff Notes

12
10.09 0.51   0.03 F6 V 25.1 -24.6 .99 -0.32 2.44 5 4402 0.001 -1.2 1 2.11 1.78 SB?
135 9.71 0.49   0.01 F5 V 23.5 -23.8 .99 -2.43 0.37 4 2567 0.615 -1.0 1 1.88 4.31  
174 11.62 0.95 0.85     27.2 -25.1 .99 -1.54 0.22 4 2629 0.383 -2.4 2 2.25 3.79 dbl
270 10.11 0.51   0.01 F7 V 22.6 -22.0 .79 +0.74 1.77 6 4402 0.000 +0.1 1 2.42 1.68 SB
299 11.19 0.64 0.56   F7 18.5 -19.0 .87 -1.82 0.48 5 4104 0.019 -2.1 1 2.10 3.92  
309 9.96 0.49   0.01 F5 V 23.4 -21.4 .86 +3.84 3.37 1     +3.1 1 3.60 -0.24  
334 10.33 0.56 0.45 0.04 F7 V 22.5 -23.1 .00 -2.47 0.72 6 4405 0.004 -2.2 2 3.94 6.41  
338 9.93 0.56   0.02 F7 V 26.5 -26.8 .96 +0.78 3.14 1     +1.2 1 3.75 2.97 dbl
350 11.13 0.71     G3 23.2 -23.0 .99 -0.55 1.16 5 5081 0.175     4.19 4.74  
361 9.68 0.44   0.01 F4 V 22.9 -22.5 .69 -2.43 0.77 4 2889 0.745 +0.5 1 3.22 5.65  
389 11.17 0.67 0.55   G0 22.5 -23.9 .99 -1.96 0.10 2 14 0.479     2.50 4.46  
453 10.39 0.62 0.53 0.12 F8 V 22.8 -23.5 .00 -5.25 6.81 3 711 0.000 -1.7 2 3.44 8.69 SB
490 9.56 0.45 0.31 0.04 F3 IV-V 23.1 -25.6 .99 -1.65 0.52 4 2885 0.182 -1.4 2 2.89 4.54  
601 11.40 0.74 0.59 0.20   22.9 -24.1 .00 -0.84 0.26 5 4065 0.960 -0.9 1      
621 9.86 0.49   0.02 F4 V 22.5 -27.0 .96 -0.51 0.67 5 4113 0.480 -1.7 2 3.33 3.84  
660 10.06 0.56 0.50 0.11 F5 V 23.1 -25.5 .99 -0.88 1.18 6 4406 0.064 -1.0 2 2.64 3.52 dbl
684 10.54 0.56 0.45 0.04 F9 V 20.6 -25.8 .98 +2.77 0.60 2 4810 0.000 -1.4 1 3.25 0.48 SB
696 11.42 0.74 0.65 0.18   19.8 -25.0 .89 -0.62 0.26 6 4065 0.221 -1.1 1      
733 9.94 0.50   0.04 F6 V 22.1 -26.6 .99 +1.79 1.59 6 4338 0.021 +0.6 1 3.31 1.52  
750 10.54 0.59   0.09 F9 V 22.0 -25.6 .99 -0.64 0.57 5 4109 0.295 +0.6 1 3.26 3.90  
767 10.66 0.60   0.08 F9 V 21.1 -26.0 .95 -0.97 0.33 5 4109 0.066 -1.5 3 2.98 3.95  
794 10.06 0.55 0.46 0.07 F3 IV-V 21.4 -24.8 .93 +2.51 3.85 4 358 0.000 +2.5 1 2.82 0.31 SB
828 11.59 0.71 0.64   F8 19.4 -26.2 .98 +0.60 0.27 4 2890 0.420 +1.0 1      
833 10.03 0.49 0.42 0.03 F6 V 22.5 -27.0 .99 +0.33 0.83 8 4109 0.025 +0.4 2      
848 9.99 0.59 0.46 0.07 F9 V 22.2 -26.4 .99 -0.26 0.22 41 4115 0.000 +3.1 2 3.66 3.92 SB2O
859 10.48 0.56 0.48 0.02 G0 23.6 -7.1 .00 +0.72 0.91 10 5225 0.000 +4.8 1     SB
863 9.21 0.52   0.02 F6 V 20.8 -27.2 .99 -23.30 4.81 1     -7.0 1 3.37   SB
917 11.10 0.70 0.57 0.19 F4 23.9 -28.3 .99 -0.08 1.12 5 4022 0.095 +1.0 1      
968 10.41 0.57   0.03 F8 V 21.1 -27.6 .99 +0.88 0.88 6 4107 0.221 -3.3 3 3.67 2.79  
988 9.80 0.56   0.07 F5 IV-V 26.8 -38.0 .99 +2.45 0.32 5 4109 0.249 +1.8 1     dbl
992 10.84 0.72 0.64 0.23 G0 15.3 -11.0 .00     1     -5.2 1     SB2
1086 11.32 0.67 0.58   G0 20.7 -24.7 .99 -1.52 0.15 1     -1.0 1 2.90 4.42  
1101 11.25 0.69 0.62   G4 20.9 -28.5 .99 -0.33 0.87 3 1924 0.368 -2.4 1 3.36 3.69  
1144 11.32 0.73     G5 32.3 -12.4   -6.57 0.15 1     +9.7 1     SB
1180 10.07 0.49 0.37   F7 20.9 -27.9 .99 -0.34 2.35 4 2983 0.004     3.81 4.25  
1185 11.19 0.72   0.19 F7 19.9 -27.9 .99 -2.15 0.97 8 5138 0.000     3.84 5.99 SB
1234 10.81 0.72 0.61   G2 21.4 -33.7 .98     1     +5.7 1 2.82   SB2
Notes: He: identification of Heckmann et al. (1956); the V, (B-V), (V-I)K and (U-B) photometry from WEBDA or Prosser et al. (1996, 1998a,b); Sp.T.: MK spectral type; $\mu_{\alpha}$, $\mu_{\delta}$: UCAC2 proper motions, Prob: membership probabilities of Fresneau (1980); $V_{\rm r}$: the mean radial velocities; $\epsilon$: error on the mean; n: number of observations; $\Delta T$: time interval of the observations; $P(\chi^2)$: probability $P(\chi^2)$; $Vr_{{\rm litt}}$: radial velocities from Stauffer et al. (1985, 1989) or Prosser (1992, 1994); N: number of spectra; Astr: astrometric radial velocity (Makarov 2006); Diff: difference with the observed radial velocity. Notes: remarks on duplicity and membership (SB: spectroscopic binary, SB2: double-lined binary; SB2O: double-lined binary with an orbit; dbl: photometric binary).


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