Contact binaries consist of two strongly interacting component stars where they are filling
their critical Roche lobes and sharing a common envelope. Most of them are main-sequence …

We present the identification and photometric analysis of 30 new low mass ratio (LMR)
totally eclipsing contact binaries found in Catalina Sky Survey data. The LMR candidates are …

DEEP, LOW MASS RATIO OVERCONTACT BINARY SYSTEMS. XIV. A STATISTICAL
ANALYSIS OF 46 SAMPLE BINARIES - IOPscience Skip to content IOP Science home …

Secondary components of W UMa-type contact binaries (CBs) have many special
properties, two of them are excess in radius and luminosity. In order to make these …

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, spectroscopic and orbital period investigations of ASASSN-V
J015428. 67+ 204247.2 (hereafter, J015428) for the first time. The light curves of VRI bands …

Using Eggleton's stellar evolution code, we study the minimum mass ratio (q min) of W
Ursae Majoris (W UMa) binaries that have different primary masses. It is found that the …

Photometric observations of the W UMa binary NSVS 2569022 are presented. The light
curve solution reveals that both components are of F spectral type (temperatures T 1= T 2 …

We present the first photometric and orbital period investigations for a neglected totally
eclipsing contact binary IP Lyn. The photometric solutions derived from both ground-based …

The first complete multicolor CCD light curves and low-resolution spectra of the short-period
Am-type eclipsing binary V2787 Ori are presented. The atmospheric parameters of the …