The improved component masses and parallaxes for the two close binary stars: HD 80671 and HD 97038

We present the fundamental stellar parameters, including the individual component masses, as well as the orbital parameters, and dynamical parallaxes of the two close binary stars; HD 80671, and HD 97038. The stellar parameters are spectrophotometrically estimated via Al-Wardat’s method for analyzing binary and multiple stellar systems, which is having a combination of the spectroscopic analysis and the photometric analysis to build the combined and individual synthetic spectral energy distributions of the individual components of the systems and so to estimate their fundamental parameters, metallicities, and ages. It employs Kurucz’s model atmospheres of single stars, while the orbital parameters are estimated using Tokovinin’s method. The individual spectrophotometric component masses are inferred with good accuracy, and found to be $M_{Sph}^A$ = 1.47$\pm 0.10M_{\odot }$ and $M_{Sph}^B=1.29\pm 0.09M_{\odot }$ with an age of $1.0\pm 0.09$ Gyr for HD 80671, and $M_{Sph}^A=1.17\pm 0.09M_{\odot }$ and $M_{Sph}^B=1.12\pm 0.08M_{\odot }$ with an age of $3.981\pm 0.35$ Gyr for HD 97038. The improved dynamical parallaxes are given as ${\pi }_{dyn}=28.305\pm 0.45$ mas for HD 80671, and ${\pi }_{dyn}=16.26\pm 0.30$ mas for HD 97038. The evolutionary status of two binaries is discussed depending on the positions of the components on the isochrones and evolutionary tracks.