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

TL;DR

This study investigates extra-mixing processes in red giant stars by measuring lithium abundance and carbon isotope ratios, providing new insights into stellar evolution beyond standard models.

Contribution

It presents observational evidence of extra-mixing in field giants using Li and 12C/13C ratios, highlighting thermohaline mixing effects and their correlation with stellar properties.

Findings

Evidence of thermohaline mixing in RGB and horizontal branch stars

Li enrichment not caused by planet engulfment

Correlations between 12C/13C, metallicity, and stellar mass

Abstract

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 associated usually with thermohaline mixing acting after the RGB bump. Peculiar Li-enriched RGB stars might also be related to either enhanced extra-mixing or pollution from external sources. We measure the Li abundance and carbon isotopic ratio 12C/13C 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. Multiple-epoch observations needed for exoplanet detection are used to decrease the effects of telluric contamination in 12C/13C measurements. 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 extra-mixing consistent with thermohaline. The most Li-enriched giant in the sample, classified as a RGB star close to the RGB bump, has low 12C/13C. Given that the 12C/13C 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 12C/13C in the RGB and an increasing correlation in the horizontal branch, which, once again, is consistent with thermohaline mixing. Our data also shows a correlation between 12C/13C and [Fe/H]. There is no evident impact of binarity either on Li or on 12C/13C. Our sample shows behavior consistent with additional mixing acting after the RGB bump. The 12C/13C adds new clues to describe extra-mixing, and could well be the best tool to study mixing in red giants. Additional measurements of 12C/13C in field stars would greatly improve our ability to compare with models and understand mixing mechanisms.