SIMBAD references

2008CoAst.153...54L - Com. in Asteroseismology, 153, 54 (2008/April-0)

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

LAMPENS P., STRIGACHEV A., KIM S.-L., RODRIGUEZ E., LOPEZ-GONZALEZ M.J., VIDAL-SAINZ J., MKRTICHIAN D., LITVINENKO D., VAN CAUTEREN P., WILS P. and GOMEZ FORELLAD J.M.

Abstract (from CDS):

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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