The Fundamental Parameters and Evolutionary Status of V454 Aurigae

Eclipsing binary systems have a unique feature, which enables scientists to obtain precise fundamental star parameters, which opens to greater area of astrophysics studies. In this study, we have derived the fundamental parameters, the evolutionary status, and the birthplace of V454 Aur in the Galaxy by combining radial velocity, photometric, and spectral energy distribution data. We have updated ephemerides and period of V454 Aur as 2458850.80136_-0.00001^ +0.00001 and 27.0198177_-0.0000003^ +0.0000003, respectively. We obtain 1.173^ +0.016_-0.016 M_⊙ and 1.203^ +0.022_-0.026 R_⊙ for the primary component and 1.045^ +0.015_-0.014 M_⊙ and 0.993^ +0.034_-0.027 R_⊙ for the secondary component. The effective temperatures for the components are accurately determined via SED data as 6250^ +150_-150 K and 5966^ +109_-89 K for the primary component and the secondary component, respectively. The metallicity of the components is derived from evolutionary tracks, which implies slightly higher than Solar metallicity. According to analysis, the components of V454 Aur are on the main sequence. Our distance calculation for the system is, which is 65.07^ +2_-3 pc, in excellent agreement with Gaia astrometric data, which is 65.07^ +0.09_-0.09 pc. The current age of the system is 1.19_-0.09^ +0.08 Gyr, and it will start to mass transfer between components in 5 Gyr from now on. Dynamical orbital analysis shows that V454 Aur follows a boxy pattern around the Galactic centre and is a member of the thin-disc component of the Galaxy. Considering the age and metallicity of this system, it was found to have formed just outside the Solar circle.