JOURNAL OF OCCULTATION AND ECLIPSE (JOE); ISSN 2522-7955; No. 6, 2019
M. Pakravanfar1, A. Poro1, I. Safaei2
1International Occultation Timing Association Middle East Section, firstname.lastname@example.org
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.
© The Author(s): This article is published with "open access" at joe.iota-me.com
Keyword: Variable star, DSLR photometry, Period, W UMa