Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...297..233b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 297, Oct. 1, 1985, p. 233-239.
Astronomy and Astrophysics
Astrophysics
16
Abundance, Carbon Stars, Giant Stars, Nitrogen, Oxygen, Stellar Composition, Cyanogen, High Resolution, Late Stars, Spectral Resolution, Spectrum Analysis, Stellar Atmospheres, Stellar Mass, Stellar Models
Scientific paper
C, N, and O abundances are presented for three giants in M67. The abundances were determined by model atmosphere analysis of high-resolution spectra of the C2 1-0 and Δυ = 0 Swan band features, the [O I] 6300 Å line, and CN red system lines. The three giants are of identical composition, except possibly for 12C/13C ratio, and are similar to low-mass giants in the field. The abundance results are log ɛ(C) = 8.3, log ɛ(N) = 8.35, and log ɛ(O) = 8.7.
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