Issue |
EAS Publications Series
Volume 64, 2013
Setting a New Standard in the Analysis of Binary Stars
|
|
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Page(s) | 331 - 338 | |
Section | Synergy: Asteroseismology of Binary Stars | |
DOI | https://doi.org/10.1051/eas/1364046 | |
Published online | 25 February 2014 |
Setting a New Standard in the Analysis of Binary Stars
K. Pavlovski, A. Tkachenko and G. Torres (eds)
EAS Publications Series, 64 (2013) 331–338
K. Pavlovski, A. Tkachenko and G. Torres (eds)
EAS Publications Series, 64 (2013) 331–338
The Dynamic Eclipse Mapping method in pulsating binaries
Baja Astronomical Observatory, Baja, Hungary
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.
© EAS, EDP Sciences, 2014