Discovery of binary systems among RR Lyrae stars belongs to challenges of
present astronomy. So far, none of classical RR Lyrae stars was clearly
confirmed that it is a part of an eclipsing system. For this reason we studied
two RR Lyrae stars, VX Her and RW Ari, in which changes assigned to eclipses
were detected in sixties and seventies of the 20th century. In this paper our
preliminary results based on analysis of new photometric measurements are
presented as well as the results from the detailed analysis of original
measurements. A new possible eclipsing system, RZ Cet was identified in the
archive data. Our analysis rather indicates errors in measurements and
reductions of the old data than real changes for all three stars.Comment: 6 pages, 4 figures, submitted to Proceedings of the 47th Conference
on Variable Stars Researc