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Mass loss rates of Li-rich AGB/RGB stars

Published online by Cambridge University Press:  30 December 2019

Walter J. Macie
Affiliation:
Astronomy Department, University of São Paulo, São Paulo, Brazil email: wjmaciel@iag.usp.br
Roberto D. D. Costa
Affiliation:
Astronomy Department, University of São Paulo, São Paulo, Brazil email: wjmaciel@iag.usp.br
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Abstract

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A sample of AGB/RGB stars with an excess of Li abundances is considered in order to estimate their mass loss rates. Our method is based on a correlation between the Li abundances and the stellar luminosity, using a modified version of the Reimers formula. We have adopted a calibration based on an empirical correlation between the mass loss rate and stellar parameters. We conclude that most Li-rich stars have lower mass loss rates compared with the majority of AGB/RGB stars, which show no evidences of Li enhancements, so that the Li enrichment process is probably not associated with an increased mass loss rate.

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