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

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22 October 2019 | 19:13


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


M. Pakravanfar1, A. Poro1, I. Safaei2
1International Occultation Timing Association Middle East Section,

2University of Kashan observatory, Kashan, Iran

 

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.

tags: W UMa Variable star DSLR photometry Period Observatory University of Kashan Observatory



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