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Bayesian analysis of ages, masses and distances to cool stars with non-LTE spectroscopic parameters

Serenelli, Aldo; Bergemann, Maria; Ruchti, Gregory R.; Casagrande, Luca

Description

For studies of Galactic evolution, the accurate characterization of stars in terms of their evolutionary stage and population membership is of fundamental importance. A standard approach relies on extracting this information from stellar evolution models

CollectionsANU Research Publications
Date published: 2013
Type: Journal article
URI: http://hdl.handle.net/1885/70937
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/sts648

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