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


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