000001973 001__ 1973
000001973 005__ 20160701171656.0
000001973 037__ $$aASTROimport-130
000001973 100__ $$aLampens, P.
000001973 245__ $$aFrequency analysis of the δ Scuti type pulsations in the semi-detachedeclipsing binary CT Her
000001973 260__ $$c2008
000001973 520__ $$aWe present the latest results of a multisite photometric campaign carried out in 2004-2007 on the Algol-type eclipsing binary system CT Her, the primary component of which is a δ Scuti- type pulsator with a main pulsation period of only 27 min. CT Her belongs to the new class of oscillating Algol-type binary systems. We collected enough data in two passbands to perform a modelling of the light curves using PHOEBE and detected up to 7 significant pulsation frequencies in the frequency range between 45-53 d-1 in the B-residual data (independent of the adopted solution for the binary model). The remaining standard deviation of the ca. 7500 B-residuals spread over 4 years is 5.0 mmag. 
000001973 700__ $$a Strigachev, A.
000001973 700__ $$a Kim, S.-L.
000001973 700__ $$a Rodriguez, E.
000001973 700__ $$a Lopez-Gonzales, M. J.
000001973 700__ $$a Vidal-Sainz, J.
000001973 700__ $$a Mkrtichian, D.
000001973 700__ $$a Litvinenko, D.
000001973 700__ $$a van Cauteren, P.
000001973 700__ $$a Wils, P.
000001973 773__ $$c328-329$$pCommunications in Asteroseismology$$v157$$y2008
000001973 85642 $$ahttp://esoads.eso.org/abs/2008CoAst.157..328L
000001973 905__ $$apublished in
000001973 980__ $$aREFERD