Scl-1013644: a CEMP-s star in the Sculptor Dwarf Spheroidal Galaxy
arXiv:1608.02252 · doi:10.1093/mnras/stw1986
Abstract
Recent studies of the Milky Way and its satellites have paid special attention to the importance of carbon-enhanced metal-poor (CEMP) stars due to their involvement in Galactic formation history and their possible connection with the chemical elements originating in the first stellar generation. In an ongoing study of red giants in the Sculptor dwarf galaxy we have discovered a star with extremely strong CN and CH molecular bands. This star, Scl-1013644, has previously been identified by Geisler et al. (2005) as a star with an enrichment in the heavy elements. Spectrum synthesis has been used to derive the carbon, nitrogen and barium abundances for Scl-1013644. Our findings are [C/Fe] = +0.8, [N/Fe] = -0.3 and [Ba/Fe] = +2.1 with the latter result consistent with the value found by Geisler et al. (2005). These results reveal Scl-1013644 as a CEMP-s star, the third such star discovered in this dwarf galaxy.
6 pages, 4 figures, 3 tables
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Cited by in corpus (7)
- Abundance analysis of a CEMP-no star in the Carina dwarf spheroidal galaxy
- Evidence for multiple nucleosynthetic processes from carbon enhanced metal-poor stars in the Carina dwarf spheroidal galaxy
- An investigation of C, N and Na abundances in red giant stars of the Sculptor dwarf spheroidal galaxy
- High-resolution spectroscopic observations of the new CEMP-s star CD-50776
- Carbon-enhanced metal-poor stars in the SDSS-APOGEE database
- Evidence of globular cluster abundance anomalies in the SMC intermediate-age cluster Kron 3
- A Main Sequence CH-star in the globular cluster M55 (NGC 6809)