ASTRONOMISCHE NACHRICHTEN, cilt.325, sa.4, ss.332-335, 2004 (SCI-Expanded)
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.