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Precise stellar mass and mass-luminosity data

Published online by Cambridge University Press:  25 May 2016

J. Andersen
J. Andersen*
Affiliation:
Astronomical Observatory; Niels Bohr Institute for Astronomy, Physics, and Geophysics; Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

Abstract

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Recent progress in observing and data reduction methods for precise mass and mass-luminosity determinations in binary systems are briefly reviewed. The foundations appear to have been laid for a new burst of accurate data. Detailed model simulations of the individual systems are the best way to use these data to critically test the theoretical models and advance our understanding of the evolution of single and binary stars.

Type
Stellar Masses and Surface Gravities
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 99 - 108
Copyright
Copyright © Kluwer 1997 

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