Accurate Light Curves of Eclipsing Binaries

Details Accurate Light Curves of Eclipsing Binaries Accurate Light Curves of Eclipsing Binaries

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mons.proc...79g&link_type=abstract

The Third MONS Workshop: Science Preparation and Target Selection, Proceedings of a Workshop held in Aarhus, Denmark, January 24

Astronomy and Astrophysics

Astrophysics

Scientific paper

Photometric observations of eclipsing binaries from space will allow the study of minor, or second-order, effects in their light curves carrying important astrophysical information. A detailed analysis of limb-darkening, gravity brightening, or reflection, currently adopted as given by theoretical approaches, will be possible and we should be prepared for it. In addition, very precise photometric observations will permit the study of perturbed stellar structure in well-detached systems as a consequence of both rotation and tides, and a better insight into their interiors will be possible through stellar oscillations, either forced by the companion or not.

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