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The non-LTE line formation of neutral carbon in late-type stars
Stockholms universitet, Naturvetenskapliga fakulteten, Institutionen för astronomi. Institutet för solfysik.ORCID-id: 0000-0002-0816-5868
2006 (Engelska)Ingår i: Astronomy & Astrophysics, ISSN 0004-6361, Vol. 458, nr 3, s. 899-914Artikel i tidskrift (Refereegranskat) Published
Abstract [en]

Aims.We investigate the non-Local Thermodynamic Equilibrium (non-LTE) line formation of neutral carbon in late-type stars in order to remove some of the potential systematic errors in stellar abundance analyses employing C i features.

Methods: .The statistical equilibrium code MULTI was used on a grid of plane-parallel 1D MARCS atmospheric models.

Results: .Within the parameter space explored, the high-excitation C i lines studied are stronger in non-LTE due to the combined effect of line source function drop and increased line opacity due to overpopulation of the lower level for the transitions considered; the relative importance of the two effects depends on the particular combination of T{eff}, log g, [Fe/H] and [C/Fe] and on the analysed C i line. As a consequence, the non-LTE abundance corrections are negative and can be substantially so, for example ˜ -0.4 dex in halo turn-off stars at [Fe/H]˜ -3. The magnitude of the non-LTE corrections is rather insensitive to whether inelastic H collisions are included or not.

Conclusions: .Our results have implications on studies of nucleosynthetic processes and on Galactic chemical evolution models. When applying our calculated corrections to recent observational data, the upturn in [C/O] at low metallicity might still be present (thus apparently still necessitating contributions from massive Pop. III stars for the carbon production), but at a lower level and possibly with a rather shallow trend of ˜ -0.2 dex/dex below [O/H]˜ -1.

Ort, förlag, år, upplaga, sidor
2006. Vol. 458, nr 3, s. 899-914
Nyckelord [en]
ine: formation, stars: abundances, stars:, late-type, Galaxy: abundances, Galaxy: evolution
Nationell ämneskategori
Astronomi, astrofysik och kosmologi Astronomi, astrofysik och kosmologi
Identifikatorer
URN: urn:nbn:se:su:diva-20164DOI: doi:10.1051/0004-6361:20065763OAI: oai:DiVA.org:su-20164DiVA, id: diva2:186689
Tillgänglig från: 2008-06-12 Skapad: 2008-06-12 Senast uppdaterad: 2019-12-04Bibliografiskt granskad

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Av författaren/redaktören
Kiselman, Dan
Av organisationen
Institutionen för astronomi
Astronomi, astrofysik och kosmologiAstronomi, astrofysik och kosmologi

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