A grid of S stars MARCS model atmospheres
2011 (English)In: Journal of Physics: Conference Series, Volume 328, 2011, 012009- p.Conference paper (Refereed)
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 (Teff, 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 V J H KL photometry are needed to disentangle the ffective 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 ffective temperature decreases.
Place, publisher, year, edition, pages
2011. 012009- p.
Astronomy, Astrophysics and Cosmology
IdentifiersURN: urn:nbn:se:uu:diva-169026DOI: 10.1088/1742-6596/328/1/012009OAI: oai:DiVA.org:uu-169026DiVA: diva2:504918
GREAT-ESF Workshop: Stellar Atmospheres in the Gaia Era