We revisited the short-period (∼ 1.5 days) binary system KIC 5444392, which shows quasi-
period modulated light variations. Previous studies indicated that these variations might be …

In the current work we present the first investigations of 14 neglected, late-type, short period
contact binaries using period variation, photometric and spectroscopic analysis performed …

We present BVR C differential photometry of an eclipsing binary system V826 Aur. A period
analysis shows near constant period of 0.36 days across two decades of observation. The …

The contact phase represents a crossroad in the evolution of massive binary stars.
Depending on the internal physics, the predicted end products can vary greatly including …

Abstract We present BVR C+ TESS differential photometry of an eclipsing binary system
NSVS 2910034. A period analysis reveals unusual variations that are inconsistent with …

Eclipsing Binaries (EBs) are known to be the source of most accurate stellar parameters,
which are important for testing theories of stellar evolution. With improved quality and …

We present a novel approach for classifying stars as binary or exoplanet using deep
learning techniques. Our method utilizes feature extraction, wavelet transformation, and a …

El estudio de las estrellas es de gran importancia para entender los bloques fundamentales
que componen el universo. En particular, los sistemas binarios eclipsantes son laboratorios …

We present a method for the inference of the minimum mass ratio of contact binary stars from
the observed distribution of their light curve amplitudes. We apply the method to a sample of …

We present BVR C differential photometry of an eclipsing binary system NSVS 4312042
using AstroImageJ. A period analysis is completed using PERANSO, and modeling is …