Li-rich AGB/RGB stars: Lithium abundances and mass loss

TL;DR

This study investigates the relationship between lithium abundances and mass loss rates in Li-rich AGB/RGB stars, finding that Li-rich stars generally exhibit lower mass loss rates than their Li-poor counterparts.

Contribution

It introduces a new method to estimate mass loss rates in Li-rich giants based on a linear relation between luminosity and lithium abundance, applied to a large stellar sample.

Findings

Li-rich stars tend to have lower mass loss rates.

A linear relation between luminosity and Li abundance is effective for estimating mass loss.

Li-rich and Li-poor stars show distinct mass loss behaviors.

Abstract

Most metal-rich AGB/RGB stars present strong Li underabundances, since this element is easily destroyed in the high temperatures of the stellar interiors. In spite of this fact, several of these stars are Li-rich, having Li abundances given by log (Li/H) + 12 > 1.5. In the present work, we extend our previous investigation on AGB/RGB stars to the expected mass loss rates of these stars. Specifically, we look for correlations between the Li abundances and the mass loss rates or related parameters in Li-rich AGB/RGB stars. We have estimated the mass loss rates using a modified form of the Reimers formula and applied it to a large sample of 104 Li-rich giant stars for which reliable stellar data are available. Our proposed method assumes a linear relation between the stellar luminosity and the Li abundance, so that the luminosity can be estimated from the Li abundance. The stellar mass is then obtained from the effective temperature and luminosity using recent evolutionary tracks. The stellar radius can be determined from the stellar gravity, so that the mass loss rate can be calculated using an adequate calibration involving both Li-rich and Li-poor stars in the AGB/RGB branches. The results show that most Li-rich stars have lower mass loss rates compared with C-rich or O-rich giants that do not present Li enhancements.