Modelling eclipsing binaries with pulsating components: Phase dependence of observed pulsation amplitudes

Details Modelling eclipsing binaries with pulsating components: Phase dependence of observed pulsation amplitudes Modelling eclipsing binaries with pulsating components: Phase dependence of observed pulsation amplitudes

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006newa...11..514r&link_type=abstract

New Astronomy, Volume 11, Issue 7, p. 514-519.

Astronomy and Astrophysics

Astronomy

2

97.80.Hn, 97.80-D, 97.30.Dg

Scientific paper

We investigate the phase dependence of the light variations due to pulsations, as modulated with light variations due to the eclipses. The study is based, both on a simplified model and on the rigorous light curve (LC) synthesis software of Wilson and Devinney. We model AB Cas as a prototype, using both of these approaches. The phase dependence of the differential light variations for total systems is also discussed .

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