Bayesian analysis of ages, masses and distances to cool stars with non-LTE spectroscopic parameters
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
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Serenelli_Bayesian_analysis_of_ages,_2013.pdf||1.76 MB||Adobe PDF||Request a copy|
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