Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
Double-lined eclipsing binaries are known to be the source of accurate stellar dimensions. Masses of radii of the component stars can be obtained with uncertainties around 1-2%, thus leading to the much-needed test of current models for stellar structure and evolution. In the present communication w...
Main Authors: | , , , , |
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Format: | |
Language: | English |
Published: |
1999
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Online Access: | http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176565 |