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The Dynamic Eclipse Mapping method in pulsating binaries

Published online by Cambridge University Press:  25 February 2014

I.B. Bíró*
Affiliation:
Baja Astronomical Observatory, Baja, Hungary
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Abstract

A short description of Dynamic Eclipse Mapping methodology is given. These tools are designed for mapping the surface patterns of non-radial oscillations on eclipsing binary components, using the effective surface sampling of the eclipses. I present two approaches to the problem, an image reconstruction (EM) and a direct model fitting (DF) method, review their capabilities and limitations, then report about the status of their application on real data, with emphasis on the encountered difficulties and caveats.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2014

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