New relationships between the orbital period and some parameters of W Ursae Majoris (W
UMa)-type systems are presented in this study. To investigate the relationships, we …

Multiband photometric investigations for eight binary systems of the W Ursae Majoris-type
are presented. Six systems are presented for the first time to analyze their light curves. All …

The accuracy of absolute parameters' estimation in contact binary systems is important for
investigating their evolution and solving some challenges. The Gaia DR3 parallax is one of …

We performed photometric and spectroscopic studies of three large amplitude contact
binaries: NSVS 2418361, ATLAS J057. 1170+ 31.2384, and NSVS 7377875. The …

Reanalyzing contact binaries with space-based photometric data and investigating possible
parameter changes can yield accurate samples for theoretical studies. We investigated light …

Asymmetries between the two maxima of the light curves of contact binaries, known as the
O'Connell effect, have been identified using the All Sky Automated Survey, All-Sky …

A lot of data in time domain were obtained by the Kepler mission, including many contact
binaries. Long-term observation lets us obtain more information about the short time scale …

Abstract Using the Kepler Eclipsing Binary Catalog, we found seven EW-type eclipsing
binaries within the tidal radius of the intermediate-aged open cluster NGC 6819 (about 40') …

We performed the first photometric study of the CSS J003106. 8+ 313347 W Ursae Majoris
(WUMa)-type system based on ground-based observations. We extracted times of minima …

Photometric data were used to perform the first light curve analysis of the V0610 Vir binary
system. We extracted the minima from our observations and compiled the literature, which …