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Home All issues Volume 507 / No 1 (November III 2009) A&A, 507 1 (2009) 541-547 Full HTML
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Table 2:

Mean radial velocities, variability, and membership.
Star HD V $\rm\langle RV \rangle$ err N P($\chi^2$) var Sp. type $v\sin i$ Membership Notes
    mag km s-1 km s-1   % const   km s-1 RV PM Adop.  
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
W3 224515 8.4 -10.8 0.4 4 97 c K0III ... n n n  
W4 224536 9.1 8.3 0.7 2 21 c F5V ... m n n  
W8   10.1 4.9 0.6 3 21 c F6III ... m n n  
W9 224630 5.6 -3.5 0.4 6 100 c K1II-III ... n n n  
W23 224820 8.4 4.8 2.2 6 27 c A1V 180 m m m  
W26 224862 7.1 17.6 0.4 4 65 c G6III ... n n n  
W28   10.5 6.7 0.6 3 26 c F2-6V ... m m m  
W32   11.1 10.7 0.7 4 24 c G8III ... n ... n  
W35 224948 10.0 7.3 0.7 3 73 c F0V 42 m m m  
W36 224964 9.0 7.3 0.5 3 23 c A3V 25 m m m  
W37 224976 9.9 2.2 0.5 23 0 v F5V 50 m? m m 1
W42 224990 5.0 5.5 0.7 95 0 v B4-5 28 m n n 2
W47   10.2 8.7 0.9 23 0 v F2V 34 m m m 2
W51 225047 8.4 6.6 2.0 5 87 c A0V 120 m m m  
W54   10.4 -4.7 0.8 4 38 c F1-5IV 43 n p n 3, 4
W55   10.7 17.3 0.9 2 43 c G0 ... n n n 5
W56   11.3 6.1 0.6 3 81 c F8 ... m m m 4
W57   10.4 7.5 6.5 17 0 v F3V 26 m? m m 2
W58   10.6 6.7 0.6 5 89 c F8V 56 m m m  
W59 225099 9.4 8.0 0.5 2 33 c F5IV-V ... m n n  
W60   10.6 6.7 0.5 5 14 c F4-6V ... m m m  
W61 225111 10.2 13.4 8.3 27 0 v F0V 28 m m m 2
W62   10.4 18.9 0.9 2 74 c G6IV ... n n n  
W63   10.6 4.6 0.4 5 36 c F4-6V ... m m m  
W65 225119 8.2 31.0 1.9 9 0 v B9: 45 n p n 6
W69 225155 7.7 -19.9 0.5 2 83 c G6III ... n n n  
W71 225187 7.1 1.9 2.8 13 0 v B7 150 ? m m?  
W74   10.5 6.6 0.5 10 53 c F6V 53 m m m  
W75 225200 6.4 14.9 5.0 12 0 v? A2shell 300: m: p m? 7
W76 225206 7.8 6.0 1.8 40 0 v B8V 146 m m m  
W80   11.0 7.7 0.6 5 26 c F6-8 ... m m m  
W86 225264 8.3 5.0 3.4 16 0 v A0-A1V 33 m m m 2
W88 225282 8.3 5.4 1.4 8 86 c A0-1 137 m m m 3
W96 50 9.7 4.5 1.9 32 0 v F0V 40 m m m  
W104 91 9.9 6.8 0.5 2 78 c F0V ... m m m 2
W106 104 8.0 -0.3 0.6 2 80 c G8-K0III ... n n n  
W109 117 9.2 15.7 0.5 4 99 c F4-8 ... n n n  
W111 141 7.9 11.4 4.4 8 100 c B9V 204 m m m  
W121 212 10.2 7.7 2.1 5 1 ? F3V 94 m m m  
W124 235 8.7 4.9 4.3 11 100 c A1V 218 m m m 3
W126 343 9.8 7.5 5.7 3 2 ? A6 155 m m m  
W128 394 9.6 3.9 1.1 2 94 c F8V 34 m n n  
E54   10.1 5.4 0.5 3 83 c F0V 28 m m m 3
E57 225077 8.9 7.5 1.2 28 0 v A3V ... m m m 2
E51   10.3 5.2 1.1 3 86 c F5V 86 m m m  

Notes: 1 the location in the color-magnitude diagram suggests duplicity (see Fig. 2); 2 binary star with calculated orbit. For kinematic membership $V_\gamma$ was used; 3 RV variability inferred from the RV difference with previous studies (see text); 4 proper motion membership taken from Mermilliod et al. (2008); 5 RV variable in Mermilliod et al. (2008); 6 suspected SB2 (see text); 7 Shell Star. RV of narrow spectral lines is constant at 6.6 $\pm$ 0.7 km s-1.


Source LaTeX | All tables | In the text

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