The sulfur abundance in HR 4049 (HD 89353)

Details The sulfur abundance in HR 4049 (HD 89353) The sulfur abundance in HR 4049 (HD 89353)

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..139t&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, Feb. 1990, p. 139-143.

Other

13

Abundance, Stellar Spectra, Sulfur, Supergiant Stars, Metallicity, Spectral Line Width, Stellar Composition, Stellar Models

Scientific paper

An abundance analysis of three S I lines at 6757, 6748, and 6743 A
observed in HR 4049 is presented. It is found that the S overabundance
derived from the S I 8694-A feature may suffer blending effects. It is
also confirmed that S is overabundant relative to other metallic
elements heavier than C, N, and O.

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