All Tables

Table 1: Our sample stars in the giant, turnoff, and lower main-sequence regions. The Strömgren photometry is from Meibom (2000), B-V from Twarog et al. (1988), and $v \sin i$ (km s^-1) from Meibom et al. (2002).
Table 2: Spectroscopic and photometric $T_{{\rm eff}}$ and [Fe/H] for the Sun and the stars in IC 4651. For the Sun, we give $\log\epsilon$ (Fe), while all cluster star abundances are relative to this value ([Fe/H]). Values in parenthesis were omitted when computing mean abundances.
Table 3: Photometric $T_{{\rm eff}}$ and associated [Fe/H] values for the rapidly rotating TO stars in IC 4651, computed with our revised reddening estimate (E(b-y) = 0.091).
Table 4: Abundance changes ( $\Delta$ [X/H]) in two stars (E60 giant, E86 main sequence) in response to variations of $T_{{\rm eff}}$ , $\log g$ , and $\xi$ ).
Table 5: Element abundances for individual solar-type dwarfs and giants in IC 4651. Entries with ":'' refer to uncertain measurements. For Cr, see text.
Table 6: Average element abundances in the sun and in IC 4651, separately for the dwarfs and giants; numbers in parenthesis gives the average number of lines used in the mean. [Ti II/Fe] is relative to the solar Fe II abundance.
Table 7: Lithium abundances for the stars in IC 4651, computed with both spectroscopic (S) and photometric (P) values of $T_{{\rm eff}}$ , assuming a reddening of E(b-y) = 0.091; we use the latter in our analysis. Asterisks indicate that W(Li) (in mÅ) refers to the unblended Li line.