Circular velocity profiles (v_c) for the MW potential model used here (black curve), and its components. We show v_c for the stellar bar and inner disk model of S22 (orange). The additional components are derived from BG16 which are: the gaseous disk (blue), the nuclear components (gray) corresponding to the Sagittarius A* super massive black hole (SMBH), the nuclear star cluster (NSC), and the nuclear stellar disk (NSD), and the dark matter halo. More details in §B. We include the v_c at Sun’s position v_c =233±7 km/s (Põder et al. 2023) at its galactocentric distance R₀ =8.2±0.1 kpc BG16. We include the axisymmetric MW potential MWPotential2014 from Bovy (2015) (gray dotted line) to compare the gravitational potential differences with our barred MW model.