Photometric solution of the eclipsing binary system EF Boötis

Details Photometric solution of the eclipsing binary system EF Boötis Photometric solution of the eclipsing binary system EF Boötis

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004an....325..332o&link_type=abstract

Astronomische Nachrichten, Vol.325, Issue 4, p.332-335

Astronomy and Astrophysics

Astronomy

Binaries: Eclipsing, Binaries: Close, Stars: Individual (Ef Bootis)

Scientific paper

The EF Boo eclipsing binary system is studied in the context of optical
light curves and radial velocity curves published in the literature. The
best-solution leads to an over-contact configuration of W-subclass of W
UMa systems with a fill-out factor of 28%. Absolute parameters based on
simultaneous solution of light and radial velocity curves are presented.

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