Physics
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...80b&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Sept.-Oct. 1990, p. 80-85. In Russian.
Physics
Carbon Isotopes, Giant Stars, K Stars, Nitrogen, Spectrum Analysis, Stellar Atmospheres, Abundance, Lithium, Metallic Stars, Stellar Interiors
Scientific paper
An N abundance of +0.6 and a C-12/C-13 ratio of 10 were determined for 9 Boo while an N abundance of -0.1 and a C-12/C-13 ratio of 12 were determined for Rho Boo. The high lithium abundance in the atmosphere of 9 Boo together with the low C/N and C-12/C-13 ratios may be interpreted as a consequence of lithium synthesis in the stellar interior during the helium core flash stage.
Bikmaev I. F.
Iakovina L. A.
Miliutikova S. V.
Pavlenko Ia. V.
Shavrina Angelina V.
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