Photometric mode identification methods in eclipsing binaries

Details Photometric mode identification methods in eclipsing binaries Photometric mode identification methods in eclipsing binaries

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.157..330l&link_type=abstract

Communications in Asteroseismology, Vol.157, p. 330-331

Computer Science

2

Scientific paper

We present a comparison of two methods developed to identify modes of nonradial pulsations in eclipsing binary stars. The first method employs the techniques of Eclipsing Mapping (EM), while the second is Direct Fitting of spherical harmonics (DF). Both methods use the effective surface sampling of the eclipses and require photometric data only. The relative merits of the methods are evaluated through tests on synthetic light curves.

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