Evidence of extra mixing in field giants as traced by the lithium and carbon isotope ratio

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dc.contributor.authorAguilera-Gomez, Claudia
dc.contributor.authorJones, Matias I.
dc.contributor.authorChaname, Julio
dc.date.accessioned2025-01-20T20:17:15Z
dc.date.available2025-01-20T20:17:15Z
dc.date.issued2023
dc.description.abstractContext. Although not predicted by standard stellar evolution, the surface abundance of light elements, such as lithium (Li), carbon, and nitrogen, changes during the red giant branch (RGB) as a result of extra mixing. This is usually associated with thermohaline mixing acting after the RGB bump. Peculiar Li-enriched RGB stars might also be related to either enhanced mixing or pollution from external sources.Aims. We measure the Li abundance and carbon isotopic ratio C-12/C-13 in a sample of 166 field red giants with -0.3 <= [Fe/H] <= 0.2, targeted by the EXPRESS radial velocity program to analyze the effects of extra mixing.Methods. We measured the abundances with spectral synthesis using high-quality spectra. Multiple-epoch observations needed for exoplanet detection were used to decrease the effects of telluric contamination in C-12/C-13 measurements.Results. Due to the prevalence of upper limits, the Li abundance pattern is complicated to interpret, but the comparison between RGB and core He-burning giants shows effects of mixing consistent with thermohaline. The most Li-enriched giant in the sample, classified as a RGB star close to the RGB bump, has low C-12/C-13. Given that the C-12/C-13 should not be affected by planet engulfment, this does not seem to be the source of the high Li. There is a decreasing correlation between mass and C-12/C-13 in the RGB and an increasing correlation in the horizontal branch, which, once again, is consistent with thermohaline mixing. Our data also show a correlation between C-12/C-13 and [Fe/H]. There is no evident impact of binarity either on Li or on C-12/C-13.Conclusions. Our sample shows behavior consistent with additional mixing acting after the RGB bump. The C-12/C-13 adds new clues which can be used to describe extra mixing, and it could well be the best tool to study mixing in giants. Additional measurements of C-12/C-13 in field stars would greatly improve our ability to compare data with models and understand mixing mechanisms.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361/202244518
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202244518
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/92385
dc.identifier.wosidWOS:000932395400007
dc.language.isoen
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectstars: evolution
dc.subjectstars: abundances
dc.titleEvidence of extra mixing in field giants as traced by the lithium and carbon isotope ratio
dc.typeartículo
dc.volumen670
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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