000001991 001__ 1991
000001991 005__ 20160701171656.0
000001991 0247_ $$2DOI$$a10.1553/cia_153s54
000001991 037__ $$aASTROimport-148
000001991 100__ $$aLampens, P.
000001991 245__ $$aA three-year photometric study of the oscillating Algol-type binary CT Her
000001991 260__ $$c2008
000001991 520__ $$aWe present the first results of a multi-site photometric campaign carried out in 2004-2006 on the Algol-type eclipsing binary system CT Her, the primary component of which is a δ Scuti-type pulsator. Our observations include (almost complete) binary light curves in the filters B and V which have been analysed following the principles of the Wilson-Devinney method. After removal of the best-matching light curve solution, the residual B and V light curves have been investigated for their pulsational content. 
000001991 700__ $$a Strigachev, A.
000001991 700__ $$a Kim, S.-L.
000001991 700__ $$a Rodríguez, E.
000001991 700__ $$a López-González, M. J.
000001991 700__ $$a Vidal-Saínz, J.
000001991 700__ $$a Mkrtichian, D.
000001991 700__ $$a Litvinenko, D.
000001991 700__ $$a van Cauteren, P.
000001991 700__ $$a Wils, P.
000001991 700__ $$a Gómez Forellad, J. M.
000001991 773__ $$c54-62$$pCommunications in Asteroseismology$$v153$$y2008
000001991 85642 $$ahttp://esoads.eso.org/abs/2008CoAst.153...54L
000001991 905__ $$apublished in
000001991 980__ $$aREFERD