Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98..783a&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, Aug. 1986, p. 783-787. Research supported by the Ci
Astronomy and Astrophysics
Astronomy
8
A Stars, Abundance, Carbon, Horizontal Branch Stars, Nitrogen, Oxygen, Infrared Spectra, Line Spectra, Red Giant Stars, Stellar Composition, Stellar Evolution
Scientific paper
From observations of infrared lines, oxygen and nitrogen abundances of the prototype field horizontal-branch stars HD 109995 and HD 161817, the somewhat similar star HD 64488, and the sharp-lined Population I A stars Theta Leo and HR 6559 have been obtained, as well as carbon abundances of HD 161817 and Theta Leo. The results for HD 161817 may be in accord with the predictions of Sweigart and Mengel (1979) for dredge-up during the previous red-giant stage if the non-LTE effects for the O I lines have been properly accounted for, and those for the C I and N I lines are small. This star and HD 109995 are apparently both oxygen and nitrogen poor to the same degree although their iron abundances differ by 0.3 dex.
Adelman Saul J.
Davis Philip A. G.
Hayes Donald S.
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