Physical dimensions and evolutionary status of the A-type twin binary GSC 4019 3345 are presented. Located at a distance of ~1.1 kpc from the Sun, the system was found to have two components with identical masses (M1,2 = 1.92 M⊙), radii (R1,2 = 1.76 R⊙), and luminosities (log L1,2 = 1.1 L⊙) revolving in a circular orbit. Modeling the components with theoretical evolutionary tracks and isochrones implies a young age (t = 280 Myr) for the system, which is bigger than the synchronization time scale but smaller than the circularization time scale. Nevertheless, synthetic spectrum models revealed components’ rotation velocity of Vrot12 = 70 km s−1, that is about three times higher than their synchronization velocity. No evidence is found for an age difference between the components.
