Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...167..111k&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 167, no. 1, Oct. 1986, p. 111-116.
Astronomy and Astrophysics
Astrophysics
16
Abundance, Binary Stars, Rare Earth Elements, Spectrum Analysis, Stellar Atmospheres, F Stars, Nuclear Fusion, Stellar Evolution
Scientific paper
A detailed abundance analysis of 13 rare-earth elements (La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Er, Tm, Yb, and Lu) has been carried out relative to the Sun for the bright F star Procyon (F5 IV - V). Weak and broadened rare-earth lines were analyzed by the method of spectrum synthesis. It was found that Procyon closely resembles the Sun in its rare-earth composition.
Kato Kazuhiro
Sadakane Koichiro
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