Theory of the light curves of eclipsing systems with oscillating components. II

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Stellar Oscillations, Angular Velocity, Asymptotic Methods, Brightness Distribution, Harmonic Oscillation

Scientific paper

The Kopal (1982c) investigation of the photometric consequences of radial or nonradial free oscillations of the eclipsing component on the light changes of close binary systems is extended to the effects of similar oscillations of the component which undergoes eclipse, with arbitrary period and phase. A theory is presented of the photometric effects caused by arbitrary harmonic oscillations of the components of eclipsing binary systems distorted by equilibrium tides, or by axial rotation with constant angular velocity. A translation of these effects into the frequency domain constitutes a problem that is solvable in a closed form only if the eclipse in question ends in totality.

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