Table 5: Data for Be 32. ID $_{\rm {phot}}$, and BVI are from D'Orazi et al. (2006), while ID $_{\rm {fla}}$ is the identification number used for FLAMES observations.
Star Star RA Dec B V I $J_{\rm {2MASS}}$ $K_{\rm {2MASS}}$ No. exp. RV S/N Notes
ID $_{\rm {fla}}$ ID $_{\rm {phot}}$                 (km s-1)    
17 533 6 58 8.242 6 24 19.48 14.754 13.667 12.540 11.683 11.028 2 105.3 80-100 M
18 997 6 58 13.762 6 27 54.89 14.730 13.661 12.534 11.709 11.069 2 105.5 80-100 M
19 787 6 58 3.089 6 26 16.08 14.800 13.709 12.564 11.722 11.024 2 101.4 70-90 M
25 121 6 57 59.819 6 26 59.93 15.387 14.242 13.028 12.153 11.450 1 105.5 45-60 M
27 605 6 58 2.262 6 24 56.71 15.511 14.372 13.177 12.282 11.607 2 105.6 60-70 M
45 1139 6 58 7.473 6 29 32.67 16.299 15.278 14.153 13.341 12.707 3 105.3 45-50 M
932 1183 6 58 1.771 6 29 55.32 14.450 13.425 12.282 11.474 10.843 2 30.8 90-100 NM
938 - 6 58 11.488 6 21 16.25 - 13.672* 12.501* 11.686 11.027 1 106.1 50-60 M
940 104 6 58 22.909 6 26 25.26 14.793 13.691 12.535 11.691 11.023 1 105.0 70-75 M
941 99 6 57 50.572 6 26 11.92 14.769 13.663 12.477 11.643 10.973 2 105.5 85-95 M


* V and I from Kaluzny & Mazur (1991).


Source LaTeX | All tables | In the text