000002062 001__ 2062
000002062 005__ 20160701171658.0
000002062 0247_ $$2DOI$$a10.1553/cia146s11
000002062 037__ $$aASTROimport-219
000002062 100__ $$aKolenberg, K.
000002062 245__ $$aOV And, a new field RRab Blazhko star?
000002062 260__ $$c2005
000002062 520__ $$aBetween 2004 November and 2005 January, we organized a small photometric observing campaign dedicated to the RRab star OV And.  This star lies very close to other stars in the field. NSVS (Northern Sky Variability Survey) data suggested the presence of the Blazhko effect in this star. The new data reveal that the large discrepancies in pulsation amplitude of the star reported in the literature can be reproduced by applying different reduction methods. We show that only the data reduced with inclusion of the neighboring stars can be considered trustworthy. Nevertheless, we find some indications that the Blazhko effect may exist in this star. 
000002062 700__ $$a Guggenberger, E.
000002062 700__ $$a Lenz, P.
000002062 700__ $$a van Cauteren, P.
000002062 700__ $$a Lampens, P.
000002062 700__ $$a Wils, P.
000002062 773__ $$c11-20$$pCommunications in Asteroseismology$$v146$$y2005
000002062 85642 $$ahttp://esoads.eso.org/abs/2005CoAst.146...11K
000002062 905__ $$apublished in
000002062 980__ $$aREFERD