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Lithium abundances in carbon-enhanced metal-poor stars

Astrophysical Journal (2012) 751(1)
DOI: 10.1088/0004-637X/751/1/14
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Abstract

Carbon-enhanced metal-poor (CEMP) stars are believed to show the chemical imprints of more massive stars (M ≳ 0.8 M ) that are now extinct. In particular, it is expected that the observed abundance of Li should deviate in these stars from the standard Spite lithium plateau. We study here a sample of 11 metal-poor stars and a double-lined spectroscopic binary with -1.8

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Masseron, T., Johnson, J. A., Lucatello, S., Karakas, A., Plez, B., Beers, T. C., & Christlieb, N. (2012). Lithium abundances in carbon-enhanced metal-poor stars. Astrophysical Journal, 751(1). https://doi.org/10.1088/0004-637X/751/1/14

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