Other
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...255..577w&link_type=abstract
Astrophysical Journal, Part 1, vol. 255, Apr. 15, 1982, p. 577-584.
Other
79
Abundance, K Stars, Late Stars, Lithium, Red Giant Stars, Resonance Lines, Stellar Atmospheres, Atmospheric Models, Carbon Isotopes, Iron, Light Elements, Metallic Stars, Nitrogen Isotopes, Oxygen Isotopes, Stellar Evolution, Stellar Spectra
Scientific paper
The strong-lined K giant star HD 112127 exhibits an extremely strong lithium resonance line in its spectrum. In most other respects the atmosphere of the star resembles the well-studied, strong-lined star Mu Leo. A model atmosphere analysis has been carried out for HD 112127 with particular emphasis on the light element abundances. Iron peak elements show essentially solar composition, while the CNO group is enhanced by about 0.2 dex. The carbon isotope ratio is near 20, while the lithium content of this star is approximately the maximum seen in unevolved stars. Schemes for the production of lithium in a relatively low luminosity giant are discussed.
Sneden Chistopher
Wallerstein George
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