Testing convection in stellar models using detached eclipsing binaries

Details Testing convection in stellar models using detached eclipsing binaries Testing convection in stellar models using detached eclipsing binaries

2006-11-16

arxiv.org/abs/astro-ph/0611525v2

Astronomy and Astrophysics

Astrophysics

3 pages, 2 figures, poster proceedings for IAUS 239 (Convection in Astrophysics). The actual poster, and other resources, can

Scientific paper

10.1017/S1743921307000336

The fundamental properties of detached eclipsing binary stars can be measured very accurately, which could make them important objects for constraining the treatment of convection in theoretical stellar models. However, only four or five pieces of information can be found for the average system, which is not enough. We discuss studies of more interesting and useful objects: eclipsing binaries in clusters and eclipsing binaries with pulsating components.

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