Astronomy and Astrophysics – Astronomy
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..574k&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, May 1990, p. 574-580. Research supported by NSF.
Astronomy and Astrophysics
Astronomy
13
Abundance, Carbon Stars, Lithium, S Stars, Stellar Spectra, Absorption Spectra, Astronomical Photometry, Cn Emission, Spectrograms, Stellar Temperature
Scientific paper
Spectra between 6685 and 6720 A have been synthesized to match high-resolution observations of eight SC stars and two S stars to study the Li 6707 A line. In addition, lines for eleven additional elements and the CN molecule were detected. Li/metals abundance ratios ranged from - 1.15 to - 1.75. The Li abundances in MS, S, and SC stars are compared with that of super-lithium-rich stars.
Kipper Tonu
Wallerstein George
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