2282 20160701171702.0 ASTROimport-439 Hambsch, F.-J. 2010 Detection of a Rapidly Pulsating Component in the Algol-Type Eclipsing Binary YY Boo The semi-detached eclipsing binary YY Boo has been found to contain a rapidly pulsating delta Scuti type component with an amplitude of 0.1 magnitude in B. A rough binary model based on BV photometry is used to disentangle the variations due to pulsation and geometric effects. Lampens, P. van Cauteren, P. Kleidis, S. Robertson, C. W. Krajci, T. Wils, P. Information Bulletin on Variable Stars 5949 2010 1 http://esoads.eso.org/abs/2010IBVS.5949....1H published in REFERD