Photometric analysis of eclipsing binary stars

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Photometric analysis of eclipsing binary stars
Published: Feb 25, 2019
DOI: https://doi.org/10.30723/ijp.v11i20.390
Keywords:
Eclipsing binaries, Photometric, PHOEBE package, BM3.

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Bushra Qassim AL-Abudi

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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How to Cite
1.
AL-Abudi BQ. Photometric analysis of eclipsing binary stars. IJP [Internet]. 2019 Feb. 25 [cited 2024 Nov. 19];11(20):120-6. Available from: https://ijp.uobaghdad.edu.iq/index.php/physics/article/view/390
Issue
Vol. 11 No. 20 (2013)
Section
Articles
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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.