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The most metal-poor stars. III. the metallicity distribution function and carbon-enhanced metal-poor fraction

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Authors

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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Source

Astrophysical Journal, The

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Open Access

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Restricted until

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