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δ Sct-type pulsations in eclipsing binary systems: RZ Cas
Authors:E. Rodrí  guez,J. M. Garcí  a,D. E. Mkrtichian,V. Costa,S.-L. Kim,M. J. Ló  pez-Gonzá  lez,E. Hintz,A. V. Kusakin,A. Y. Gamarova,J. W. Lee,J.-H. Youn,E. B. Janiashvili,R. Garrido,A. Moya, Y. W. Kang
Affiliation:Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, E-18080 Granada, Spain;Departamento de Física, E.U.I.T. Industrial, UPM, Ronda de Valencia 3, E-28012 Madrid, Spain;Astrophysical Research Center for the Structure and Evolution of the Cosmos (ARCSEC), Sejong University, Seoul 143-747, Korea;Astronomical Observatory, Odessa National University, Shevchenko Park, Odessa, 65014, Ukraine;Korea Astronomy Observatory, Daejeon 305-348, Korea;Department of Physics and Astronomy, Brigham Young University, Provo, UT 84602, USA;Sternberg State Astronomical Institute, Universitetsky prospect, 13, Moscow, 119899, Russia;Isaac Newton Institute in Chile, Kazakhstan Branch;Abastumani Astrophysical Observatory, Abastumani, 383763, Georgia
Abstract:
Keywords:techniques: photometric    binaries: eclipsing    stars: individual: RZ Cas    stars: oscillations    δ Scuti
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