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

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

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ibvs.5949....1h&link_type=abstract

Information Bulletin on Variable Stars, 5949, 1.

Computer Science

2

Ccd Photometry

Scientific paper

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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