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Paper: On the Surface Temperature-Gravity-Mass Relation of H-Deficient Post-AGB Tracks
Volume: 378, Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes
Page: 131
Authors: Miller Bertolami, M.M.; Althaus, L.G.; Weiss, A.
Abstract: We explore whether the systematic difference between asteroseismological and spectroscopic masses in PG1159–type stars can be understood in terms of uncertainties in mass-loss rates and/or third dredge-up efficiencies in the TP–AGB. We find that neither of them can account for the discrepancy.
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