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Observational evidence of interacting processes in the system TW Draconis

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TW Draconis is one of the best studied Algol-type eclipsing binaries. There is significant evidence for miscellaneous interacting physical processes between binary components and these are manifested in period and light curve changes. We studied these processes on the basis of a long-time series of photometric and spectroscopic observations.
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Keywords: Close binaries; Eclipsing binaries; Short-time variations in oscillations; TW Dra

Document Type: Research Article

Affiliations: Institute of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic

Publication date: 2007-02-01

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