Photometry and Light Curve Modeling of HO Piscium and V535 Pegasi

Volume 46 number 2 (2018)

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Rahim Heidarnia
RIAAM Observatory, Research Institute for Astronomy and Astrophysics of Maragha, Maragha, Iran; heidarnia.rahim@gmail.com

Abstract

In this article we will present the photometric study of the overcontact binaries HO Psc and V535 Peg. The data were acquired with the 304-mm telescope of RIAAM Observatory, and after the data reduction and photometry, the main parameters of the systems such as temperatures, inclination, and mass ratio were found using modeling in phoebe software.