EDP Sciences
Free Access
Volume 501, Number 3, July III 2009
Page(s) 965 - 971
Section Galactic structure, stellar clusters, and populations
DOI https://doi.org/10.1051/0004-6361/200811194
Published online 19 May 2009

Online Material

Table 1:   Stellar objects used in this study, their coordinates, V magnitude, and the projected rotational velocity $\upsilon\sin{i}$. High probability members proposed for the different associations are identified with an H in the last column. The remaining stars are possible members (P).

Table 2:   The determined atmospheric parameters $T_{\rm eff}$, $\log ~g$, [Fe/H], $\xi _{\rm t}$ for each star. In the last three columns, we show the number of Fe lines used in each determination, the average uncertainty in the abundances given by each line EW.

Table 5:   Derived abundances of Si and Ni for the stars in the sample.

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