Mode Identification of Nonradial Pulsations by Image Reconstruction in Eclipsing Binary Systems

Details Mode Identification of Nonradial Pulsations by Image Reconstruction in Eclipsing Binary Systems Mode Identification of Nonradial Pulsations by Image Reconstruction in Eclipsing Binary Systems

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..333..221b&link_type=abstract

Tidal Evolution and Oscillations in Binary Stars: Third Granada Workshop on Stellar Structure, ASP Conference Series, Vol. 333,

Astronomy and Astrophysics

Astronomy

9

Scientific paper

We have developed a method adapted to the reconstruction of dynamical surface structures with known temporal behaviour. Nonradially pulsating components of eclipsing binaries are genuine samples of such time dependent features and we present test reconstructions of the modulation patterns in a simulated binary system of this kind. This technique allows a pure geometric approach to the mode identification and may allow a deeper analysis of these systems as compared to single pulsating stars.

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