Sulphur in the Sculptor dwarf spheroidal galaxy - Including NLTE corrections
arXiv:1505.03155 · doi:10.1051/0004-6361/201525956
Abstract
In Galactic halo stars, sulphur has been shown to behave like other -elements, but until now, no comprehensive studies have been done on this element in stars of other galaxies. Here, we use high-resolution ESO VLT/FLAMES/GIRAFFE spectra to determine sulphur abundances for 85 stars in the Sculptor dwarf spheroidal galaxy, covering the metallicity range . The abundances are derived from the S~I triplet at 9213, 9228, and 9238~Å. These lines have been shown to be sensitive to departure from local thermodynamic equilibrium, i.e. NLTE effects. Therefore, we present new NLTE corrections for a grid of stellar parameters covering those of the target stars. The NLTE-corrected sulphur abundances in Sculptor show the same behaviour as other -elements in that galaxy (such as Mg, Si, and Ca). At lower metallicities () the abundances are consistent with a plateau at , similar to what is observed in the Galactic halo, . With increasing [Fe/H], the [S/Fe] ratio declines, reaching negative values at . The sample also shows an increase in [S/Mg] with [Fe/H], most probably because of enrichment from Type Ia supernovae.
9 pages, 11 figures, 2 tables + 3 online tables, accepted in A&A
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