The photometry of the binary star BX And (HIP 10027) is performed during
several nights in October and November 2019, and October 2020 using B, V,
and R Johnson-Cousins filters in Dr. Mojtahedi Observatory of the University
of Birjand. Astronomical image processing and data reduction are performed
by the IRIS software and light curves are obtained. These curves, along with
the radial velocity data of the binary star, are analyzed by the Phoebe
program to determine the physical and geometric parameters of the system.
The evolutionary state of this system is investigated using the
Hertzsprung-Russell (H-R) and density vs color index diagrams. The O-C curve
is plotted using the eclipse times obtained in this study and those reported
in the literature. By fitting a quadratic function to this curve, a new
linear ephemeris is obtained for the system, and the mass transfer rate
between the components of the system is determined. A periodic behavior is
observed in the residuals, after subtracting the quadratic function from the
O-C curve. These periodic changes are attributed to the presence of a third
component in the system. The parameters of the third component are
determined by fitting the light-time function to the residuals curve.