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New Light Curves and Ephemeris of W UMa-type binary star BX Pegasi

Abstract : In this article, the new light curve of W UMa type eclipsing binary star BX Peg is presented. The observations were made at the University of Kashan Observatory by DSLR camera method in Clear filter. The new light curve, times of minima and period were calculated, and finally, the O-C diagram was drawn by previous information and the new calculation in this project.
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https://hal.archives-ouvertes.fr/hal-02314267
Contributor : Atila Poro <>
Submitted on : Saturday, October 12, 2019 - 4:01:07 AM
Last modification on : Monday, October 14, 2019 - 3:24:25 PM
Document(s) archivé(s) le : Monday, January 13, 2020 - 12:41:03 PM

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  • HAL Id : hal-02314267, version 1

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M Pakravanfar, A. Poro, I Safaei. New Light Curves and Ephemeris of W UMa-type binary star BX Pegasi. JOE - Journal of Occultation and Eclipse, IOTA/ME, 2019. ⟨hal-02314267⟩

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