uvby-beta photometry of metal-poor stars
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Using the calibrations derived by Schuster and Nissen (=1989A&A...221...65S), the interstellar color excesses, E(b-y), and the metallicities, [Fe/H], have been determined...
基于Schuster与Nissen（1989A&A...221...65S）推导得到的定标结果，星际色余（interstellar color excess）E(b-y)与金属丰度（metallicity）[Fe/H]已被测定……
