Abstract
Very metal-poor stars are of obvious importance for many problems in chemical evolution, star formation, and galaxy evolution. Finding complete samples of such stars which are also bright enough to allow high-precision individual analyses is of considerable interest. We demonstrate here that stars with iron abundances [Fe/H]
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Fulbright, J. P., Wyse, R. F. G., Ruchti, G. R., Gilmore, G. F., Grebel, E., Bienaymé, O., … Zwitter, T. (2010). The RAVE survey: Rich in very metal-poor stars. Astrophysical Journal Letters, 724(1 PART 2). https://doi.org/10.1088/2041-8205/724/1/L104
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