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Abstract WIYN/Hydra spectroscopy (at R ∼ 15,000) of the moderately metal-rich Praesepe and Hyades open clusters was used to study their main-sequence (MS) iron (Fe/H) and lithium ( A (Li)) abundances. Self-consistent Fe/H and Li analyses of these clusters of consistent age, which we re-evaluate, confirms that they have consistent Fe/H and provides a foundation to investigate the poorly understood G-dwarf and F-dwarf Li-depletions. Neither phenomenon agrees with standard stellar evolution theory, but possible explanations abound. We supplement our A (Li) with previously published results placed on a uniform abundance scale. This creates the largest self-consistently analyzed sample of A (Li) in both the Hyades (90) and Praesepe (110). For each star, high-precision UBVRI photometry was used to determine a 10-color-based and then to test for photometric peculiarities indicated by a large (>75 K). The stars that have large were predominantly found to be binaries or stars with peculiar (apparent) A (Li). When considering only proper-motion members that have low and are also photometrically consistent with the cluster MS fiducial, each cluster has a more tightly defined Li morphology than previously observed and the two clusters’ A (Li) are indistinguishable. This suggests that clusters of consistent age and metallicity may have consistent Li-depletion trends across a broad range of no additional major parameters are required, at least for these two clusters. We propose that the combined Hyades and Praesepe data offer more rigorous constraints than does either cluster alone, and we discuss newly revealed features of the combined Li– trend.
Cummings et al. (Thu,) studied this question.