Light Curve Analysis of GSC 2750-0054 and GSC 03208-02644

TL;DR

This paper presents the first photometric analysis of two newly discovered Algol-type eclipsing binaries, determining their physical parameters, spectral classifications, and distances using Wilson Devinney code and evolutionary models.

Contribution

It introduces the first detailed photometric analysis of GSC 2750-0054 and GSC 03208-02644 using advanced modeling techniques.

Findings

Determined physical parameters and spectral types of the binary components.

Calculated distances to both systems based on photometric solutions.

Compared observational data with stellar evolutionary models.

Abstract

We present the first photometric analysis for the newly discovered eclipsing binary systems of Algole-type GSC 2750-0054 and GSC 03208-02644. Our analysis was carried out by means of the most recent version of Wilson Devinney (WD) code, which applies the model atmosphere by Kurucz (1993) with prescription in pass band for the radiative treatment. The accepted light curve solutions reveal absolute physical parameters and the spectral classifications for the components are adopted. Distance to each system was calculated based on the parameters of the accepted photometric solutions. Comparison with the evolutionary models are presented.