Population studies. XIII. A new analysis of the Bidelman-Macconnell "weak-metal" stars - Confirmation of metal-poor stars in the thick disk of the galaxy
A new set of very high signal-to-noise (S/N > 100/1), medium-resolution (R ∼ 3000) optical spectra have been obtained for 302 of the candidate "weak-metal" stars selected by Bidelman & MacConnell. We use these data to calibrate the recently devel
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Beers_Population_studies._XIII._A_2014.pdf||871.43 kB||Adobe PDF|
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