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A grid of S stars MARCS model atmospheres
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2011 (English)In: Journal of Physics, Conference Series, ISSN 1742-6588, E-ISSN 1742-6596, Vol. 328, 012009- p.Article in journal (Refereed) Published
Abstract [en]

S stars are cool stars of temperatures similar to those of M giants, but their atmospheres are enriched in carbon and s-process elements because of either extrinsic pollution by a binary companion or intrinsic nucleosynthesis and dredge-up on the thermally-pulsing AGB. Despite numerous attempts to link phenomenological spectral classification criteria to physical parameters (T$_eff$, gravity, C/O, [s/Fe], [Fe/H]), the parameter space of S stars is poorly known and this has prevented accurate abundance analysis of S stars until now. Here we present a large grid of S-star model atmospheres. ZrO and TiO band strength indices as well as VJHKL photometry are needed to disentangle the effective temperature, C/O and [s/Fe]. The stellar parameters derived on the basis of low-resolution spectra and photometry are shown to be fairly accurate when compared to high-resolution data of the same stars. The C/O ratio of S stars is found to be between the solar value (0.5) and 0.99, and not 1 as often claimed in the literature. Consistently with stellar evolution expectations, the C/O ratio increases as the effective temperature decreases.

Place, publisher, year, edition, pages
2011. Vol. 328, 012009- p.
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Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-169741DOI: 10.1088/1742-6596/328/1/012009OAI: oai:DiVA.org:uu-169741DiVA: diva2:507837
Available from: 2012-03-06 Created: 2012-03-05 Last updated: 2017-12-07Bibliographically approved

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Edvardsson, BengtEriksson, KjellGustafsson, Bengt

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