HE 0557−4840: Ultra–Metal‐Poor and Carbon‐Rich

Abstract

We report the discovery and high-resolution, high-S/ N spectroscopic analysis of the ultraYmetal-poor red giant HE 05574840, which is the third most heavy-elementYdeficient star currently known. Its atmospheric parameters are T eA 4900 K, log g 2:2, and Fe/ H 4:75. This brings the number of stars with Fe/ H < 4:0 to three, and the discovery of HE 05574840 suggests that the metallicity distribution function of the Galactic halo does not have a ''gap'' between Fe/H 4:0, where several stars are known, and the two most metal-poor stars, at Fe/ H $ 5:3. HE 05574840 is carbon rich (C/ Fe 1:6), a property shared by all three objects with Fe/ H < 4:0, suggesting that the well-known increase of carbon relative to iron with decreasing [Fe/ H ] reaches its logical conclusion (ubiquitous carbon richness) at lowest abundance. We also present abundances (nine) and limits (nine) for a further 18 elements. For species having well-measured abundances or strong upper limits, HE 05574840 is ''normal'' in comparison with the bulk of the stellar population at Fe/ H $ Y4:0, with the possible exception of Co. We discuss the implications of these results for chemical enrichment at the earliest times, in the context of single-(''mixing and fallback'') and two-component enrichment models. While neither offers a clear solution, the latter appears closer to the mark. Further data are required to determine the oxygen abundance and improve that of Co, and hence more strongly constrain the origin of this object.