A three-year photometric study of the oscillating Algol-type binary CT Her

Details A three-year photometric study of the oscillating Algol-type binary CT Her A three-year photometric study of the oscillating Algol-type binary CT Her

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.153...54l&link_type=abstract

Communications in Asteroseismology, Vol.153, p. 54-62

Computer Science

5

Scientific paper

We present the first results of a multi-site photometric campaign carried out in 2004-2006 on the Algol-type eclipsing binary system CT Her, the primary component of which is a δ Scuti-type pulsator. Our observations include (almost complete) binary light curves in the filters B and V which have been analysed following the principles of the Wilson-Devinney method. After removal of the best-matching light curve solution, the residual B and V light curves have been investigated for their pulsational content.

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