000001964 001__ 1964
000001964 005__ 20160701171656.0
000001964 0247_ $$2DOI$$a10.1051/0004-6361:20034543
000001964 037__ $$aASTROimport-121
000001964 100__ $$aArentoft, T.
000001964 245__ $$aOn the δ Scuti star in the eclipsing binary WX Eridani
000001964 260__ $$c2004
000001964 520__ $$aWX Eri is an eclipsing binary system for which one component was reported to show δ Scuti type pulsations with periods close to integer fractions of the orbital period. This makes it an interesting candidate for investigating the interaction between binarity and pulsation and a potential new member of the recently defined group of mass-accreting pulsating components (gainers) in semi-detached Algol binaries called ``oscillating EA'' stars. We present new photometric time-series observations of this star. The Wilson-Devinney code was applied to find the best fitting model for the eclipsing binary's light curve. The aim of the observations was to investigate the short-period δ Scuti type pulsations of WX Eri. However, no evidence for the presence of such oscillations was found in our data. Based on observations obtained at the South African Astronomical Observatory, ESO, Las Campanas, Beersel Hills, Hoher List and Esteve Duran Observatories. Table 2 is available in electronic form via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/418/249 
000001964 700__ $$a Lampens, P.
000001964 700__ $$a Van Cauteren, P.
000001964 700__ $$a Duerbeck, H. W.
000001964 700__ $$a García-Melendo, E.
000001964 700__ $$a Sterken, C.
000001964 773__ $$c249-254$$pAstronomy and Astrophysics$$v418$$y2004
000001964 85642 $$ahttp://esoads.eso.org/abs/2004A%26A...418..249A
000001964 905__ $$apublished in
000001964 980__ $$aREFERD