The most metal-poor stars. III. the metallicity distribution function and carbon-enhanced metal-poor fraction
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
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Yong_The_most_metal-poor_stars._2013.pdf||724.37 kB||Adobe PDF|
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