Apsidal rotation in the eclipsing binary AG Persei

Details Apsidal rotation in the eclipsing binary AG Persei Apsidal rotation in the eclipsing binary AG Persei

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.129..187w&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 129, no. 1, Jan. 1987, p. 187-193. NSF-NASA-supported research.

Astronomy and Astrophysics

Astrophysics

6

Apsides, Eclipsing Binary Stars, Light Curve, Spectrum Analysis, Stellar Rotation, Orbital Elements, Radii

Scientific paper

New three-filter light curves of AG Per are given. These yield times of minimum light in accord with the known rate of apsidal rotation but do not improve that rate. These light curves and all other published historical ones have been treated with the code EBOP and are shown to give largely consistent geometric and photometric parameters no matter which orientation of the orbit is displayed to the observer.

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