Photometric analysis of eclipsing binary stars
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Abstract
In this paper, photometric analysis of two short period group of the eclipsing binaries (RS CVn); RT And and BH Vir is presented. New physical and geometric parameters were obtained by performing two computer modeling. The first model is software package PHOEBE based on the Wilson–Devinney method, and the second is Binary Maker 3 (BM3).Our results are in good agreement with those obtained using the same modeling.
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AL-Abudi BQ. Photometric analysis of eclipsing binary stars. IJP [Internet]. 2019 Feb. 25 [cited 2024 Dec. 19];11(20):120-6. Available from: https://ijp.uobaghdad.edu.iq/index.php/physics/article/view/390
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© 2023 The Author(s). Published by College of Science, University of Baghdad. This is an open-access article distributed under the terms of the Creative Commons Attribution 4.0 International License.