BSN: First Light Curve Study of the Low Mass Contact Binary V0610 Vir

TL;DR

This study presents the first light curve analysis of the low-mass contact binary V0610 Vir, revealing its physical parameters and system characteristics using photometric data and advanced modeling techniques.

Contribution

It introduces the first detailed light curve analysis of V0610 Vir, utilizing the BSN project data, PHOEBE modeling, and MCMC approach to determine its properties.

Findings

V0610 Vir is a low-mass contact binary with a fillout factor of 0.085.

The system has a mass ratio of 0.998 and an inclination of 70.65 degrees.

The total mass of the system is estimated to be less than 0.8 solar masses.

Abstract

Photometric data were used to perform the first light curve analysis of the V0610 Vir binary system. Observations and analysis were done in the form of the Binary Systems of South and North (BSN) Project. We extracted the minima from our observations and compiled the literature, which was few. Therefore, we performed computations using the reference ephemeris and presented a new ephemeris and O-C diagram with a linear fit. Light curve analysis was performed using the PHOEBE Python code and the Markov chain Monte Carlo (MCMC) approach. The assumption of a hot starspot was required due to the asymmetry in the light curve's maxima. The analysis shows that V0610 Vir is a contact binary system with a fillout factor of 0.085, a mass ratio of 0.998, and an inclination of 70.65-deg. The absolute parameters of the system were estimated based on the Gaia DR3 parallax method. The results show that the system is a low-mass contact binary with a total mass lower than 0.8(M_Sun). The location of the stars was shown in the M-L and M-R diagrams.