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Home All issues Volume 501 / No 2 (July II 2009) A&A, 501 2 (2009) 553-562 Full HTML
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Table 1:

Sample stars: the first eight stars (R1-W79) are members of IC 2602, while the remaining seven belong to IC 2391.
Star Inst. Exp.time S/N V B-V $T_{\rm eff}$ $v\sin{i}$
    (s)       (K) (km s-1)
(1) (2) (3) (4) (5) (6) (7) (8)
R1 UVES $5 \times 870$ 200 11.6 0.91 5050 $\leq$10
R14 UVES $5 \times 870$ 230 11.6 0.87 5150 13
R15 UVES $10 \times 870$ 200 11.7 0.93 4810 7
R66 UVES $4 \times 860$ 220 11.1 0.68 5560 12
R70 UVES $5 \times 900$ 250 10.9 0.69 5700 12
R92 UVES $7 \times 300$ 200 10.3 0.69 5630 14
R95 CASPEC 1200 150 11.7 0.87 5020 12
W79 RLCeS 900 100 11.6 0.83 5260 8
VXR3 UVES $5 \times 900$ 260 10.9 - 5590 10
VXR31 UVES $7 \times 900$ 280 11.2 - 5630 17
VXR67 UVES $8 \times 870$ 130 11.7 - 4750 8
VXR70 UVES $5 \times 900$ 260 10.8 0.64 5557 17
VXR72 UVES $8 \times 900$ 250 11.5 0.73 5260 15
VXR76a RLCeS 900 70 12.8 1.05 4400 8
SHJM2 UVES $7 \times 300$ 270 10.3 0.57 5970 $\leq$15
(1) Identifier from Randich et al. (1995) for IC 2602 stars with the exception of W79 (Whiteoak 1961), and from Patten and Simon (1996) for IC 2391 members; (2) instruments (UVES, CASPEC and Red Long-Camera echelle spectrograph -RLCeS); (3) exposure time and number of exposures; (4) S/N ratios at 6707.78 Å; (5) V magnitude from Randich et al. (2001); (6) B - V colors from Randich et al. (2001); (7) initial $T_{\rm eff}$ from Randich et al. (2001), and (8) $v\sin{i}$ from Stauffer et al. (1997).

Source LaTeX | All tables | In the text

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