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The sulfur abundance in HR 4049 (HD 89353)
1990
Publications of the Astronomical Society of the Pacific
The abundance analysis of three S I lines at 6757 Â, 6748 Â, and 6743 Â observed in HR 4049 reveals that the S overabundance derived from the S I 8694 A feature may suffer blending effects and confirms that S is overabundant relative to other metallic elements heavier than C, N, and O.
doi:10.1086/132619
fatcat:avd3o2fq4nh55hh3tfqphe5e5i