The most metal-poor stars. III. the metallicity distribution function and carbon-enhanced metal-poor fraction
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Yong, David
Norris, John
Bessell, Michael
Christlieb, N
Asplund, Martin
Beers, Timothy C
Barklem, Paul S
Frebel, Anna
Ryan, Sean G
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IOP Publishing
Abstract
We examine the metallicity distribution function (MDF) and fraction of carbon-enhanced metal-poor (CEMP) stars in a sample that includes 86 stars with [Fe/H] ≤ -3.0, based on high-resolution, high signal-to-noise spectroscopy, of which some 32 objects l
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Astrophysical Journal, The
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