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Carbon-Enhanced Metal-Poor Stars in SDSS/SEGUE Cumulative frequencies of CEMP stars ([C/Fe] ≥ +0.7) from the SDSS/SEGUE sample, as a function of [Fe/H], for three different luminosity classes: giants (circles), main-s
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Document Date: 2014-03-07 10:40:33
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File Size: 403,01 KB
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