All Tables

• Table 1: The program stars, listed according to their HD numbers. The effective temperature and gravity of the Kurucz model used in the present abundance analysis. The last column indicates the category to which the objects belong. References: ^a Backman & Paresce (1993), ^b Bhatt & Manoj (2000), ^c Coulson et al. (1998), ^d Kalas et al. (2002), ^e Malfait et al. (1998a), ^f Patten & Willson (1991), ^g Song et al. (2000), ^h Thé et al. (1994).
• Table 2: The solar abundances for C, N, O and S are respectively 8.56, 8.05, 8.93 and 7.21 dex (Anders & Grevesse 1989). The given error represents the line-to-line scatter. The number of lines that were used in the abundance determination is mentioned in parentheses.
• Table 3: The abundances of the "metals''. The adopted solar abundances for Mg, Si, Ca, Ti, Fe and Sr are respectively 7.58, 7.55, 6.36, 4.99, 7.52 and 2.90 dex (Anders & Grevesse 1989). The given error represents the line-to-line scatter. The number of lines that were used in the abundance determination is mentioned in parentheses.
• Table 4: The abundances of other elements. The adopted solar abundances for Na, Al, Sc, V, Cr, Mn, Ni, Zn, Y, Zr and Ba are respectively 6.33, 6.47, 3.10, 4.00, 5.67, 5.39, 6.25, 4.60, 2.24, 2.60 and 2.13 dex (Anders & Grevesse 1989). The given error represents the line-to-line scatter. The number of lines that were used in the abundance determination is mentioned in parentheses. Two numbers refer to the neutral and first ionization state of the element, respectively.
• Table 5: The projected rotational velocity.