Ref: ASTROimport-439

Detection of a Rapidly Pulsating Component in the Algol-Type Eclipsing Binary YY Boo

Hambsch, F.-J. ; Lampens, P. ; van Cauteren, P. ; Kleidis, S. ; Robertson, C. W. ; Krajci, T. ; Wils, P.

published in Information Bulletin on Variable Stars, 5949, pp. 1 (2010)

Abstract: 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.

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The record appears in these collections:
Royal Observatory of Belgium > Astronomy & Astrophysics
Science Articles > Peer Reviewed Articles

 Record created 2016-07-01, last modified 2016-07-01