Table 3: Mean radial and rotational velocities for non-member stars.
No. V B-V U-B SpT $V_{\rm r}$ $\epsilon$ n $\Delta T$ $P(\chi^2)$ $V \sin i$ Err Rem
6 8.79 0.50 -0.05 F9 V -24.63 0.18 6 3632 0.745 2.7 1.4  
35 8.37 0.41 0.03 F6 V -2.49 0.29 39 1138 0.000 21.1 4.0 SB2O
74 8.56 0.56   G5 -6.58 0.15 8 5119 0.650 7.9 0.6  
127 8.80 0.54 0.04 F8/9 V -19.97 0.23 8 7539 0.025 7.3 0.6  
135 10.10 0.91 0.60 G8 III +21.08 0.15 6 5463 0.743 3.2 1.1  
142 9.96 0.65 0.13 G5 +8.52 0.21 4 2589 0.975 1.9 1.9  
147 8.58 0.55 0.02 F6 IV-V -13.68 0.26 19 3565 0.000 21.7 2.2 SB2O
203 10.79 0.87 0.57 G9 V -14.57 0.17 5 5434 0.844 0.0 0.0 Tr A3
214 10.00 0.79 0.33 G9 V +62.44 0.19 5 5454 0.400 4.0 1.4 Tr A14
219 11.18 0.82 0.39 G9 V -16.26 0.20 5 5789 0.713 1.9 1.8 Tr A19
221 10.37 0.82 0.41 G7 V +30.51 0.22 5 5454 0.220 3.0 1.7 Tr A21
222 11.26 0.98     -44.59 0.15 7 4363 0.880 1.1 1.5 Tr B1
275 10.82 0.95 0.74 K1 V -6.92 0.87 15 3564 0.000 4.5 0.6 Argue 8-21, SB
280 11.49 0.90 0.57 G8 III -4.36 0.18 5 5431 0.803 1.8 1.6 Argue 9-10
293 11.70 0.94 0.55 G8 III -1.31 0.19 5 5082 0.894 3.0 1.9 Argue 10-21
299 12.38 1.14 1.21   -25.49 0.25 3 3628 0.688 1.3 3.9 Argue 11-24
311 10.47 0.71 0.27   -50.24 0.29 5 5454 0.049 0.8 2.6 Argue 13-18
334 11.61 0.88 0.54 G8 III +13.68 0.21 4 5813 0.686 2.8 0.0 Argue 15-16
351 12.33 1.00 0.57 K0 +41.71 0.27 3 3628 0.492 0.0 0.0 Argue 17-14
379 11.65 1.26 1.24 K2 V -5.73 0.70 4 3183 0.000 2.3 1.8 Argue 19-28, SB
386 8.08 0.41   F5 V +6.83 2.29 3 617 0.196 66.8 7.8 Bou 38
414 12.01       +10.18 0.24 3 1455 0.390 1.9 0.0 Malm 24.292
415 12.18       -6.80 0.95 3 1455 0.000 5.1 3.3 Malm 24.314, SB
416 10.51 0.79   G8 III +12.45 5.75 5 4319 0.000 1.1 0.0 Malm 25.055, SB2O
417 11.32 1.05     +79.27 0.29 4 4419 0.105 0.0 0.0 Malm 25.141
418 11.51 1.03   G8 III +75.07 0.20 4 3688 0.856 2.8 0.0 Malm 26.078
422 11.23 1.04   K0 III +14.78 0.22 4 4427 0.371 2.7 0.0 Malm 26.250
423 11.12 1.05   K0 III +74.81 2.68 4 4427 0.000 0.0 0.0 Malm 26.286, SB
424 10.91 0.96   K3 V -15.76 0.19 5 5459 0.341 3.7 1.3 Malm 26.364
425 10.24 0.76   G5 +14.54 0.17 5 3982 0.395 2.1 1.6 Malm 26.392
427 11.72 1.08   G8 V +12.36 0.22 4 4401 0.652 2.6 2.3 Malm 27.297
428 11.74       +10.09 0.55 13 4366 0.000 7.9 1.6 Malm 27.506, SB
430 11.22 0.92   K0 III -30.10 0.20 4 4432 0.898 1.1 2.7 Malm 28.108
432 11.51     K1 V +7.66 0.25 5 4340 0.126 3.1 1.6 Malm 28.345
433 10.13       -16.20 10.50 4 3980 0.000 1.6 2.2 Malm 28.351, SB2O
434 10.67 0.87   G8 III -15.87 0.18 5 3984 0.965 1.7 0.0 Malm 30.178
435 10.07 0.71   G5 -14.86 0.48 7 5100 0.000 4.8 1.7 Malm 30.179, SB
437 9.10 0.45   G0 -4.05 2.07 7 2063 0.000 9.4 0.5 Bou 49, SB
Notes: stellar identification, according to Trumpler (1938) and extension in WEBDA, V, B-V, and U-B photometric indices, spectral types, CORAVEL mean radial velocities and errors in km s-1, the number of observations, probability $P(\chi^2)$ that the scatter is due to random errors, projected rotation ($V \sin i$) and error, also in km s-1, and remarks on binarity and cross-identifications.

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