On the Surface Temperature-Gravity-Mass Relation of H-Deficient Post-AGB Tracks

Details On the Surface Temperature-Gravity-Mass Relation of H-Deficient Post-AGB Tracks On the Surface Temperature-Gravity-Mass Relation of H-Deficient Post-AGB Tracks

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..131m&link_type=abstract

Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes. ASP Conference Series, Vol. 378, proceedings of the co

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Scientific paper

We explore whether the systematic difference between asteroseismological
and spectroscopic masses in PG 1159--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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