Volume 501, Number 3, July III 2009
|Page(s)||965 - 971|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||19 May 2009|
Table 1: Stellar objects used in this study, their coordinates, V magnitude, and the projected rotational velocity . 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 , , [Fe/H], 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.
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