The temperature discrepancy factor (f T ≡ T w/T adi) as a function of the metallicity (﹩\hat{Z}\equiv Z/﹩ Z⊙ = 1, 0.5, 0.25, and 0.125), the mass-loss rate (﹩\mathrm{log}{\dot{M}}_{\mathrm{sc}}=-1﹩, −2, −3, and −4 M ⊙ yr−1 at Z = Z⊙) coupled to the metallicity (﹩{\dot{M}}_{\mathrm{sc}}\propto {Z}^{0.72};﹩ see Table 1), and the wind terminal velocity (V ∞ = 250, 500, and 1000 km s−1 at Z = Z⊙) coupled to the metallicity (V ∞ ∝ Z 0.13; see Table 1), and the ambient density (﹩\mathrm{log}{n}_{\mathrm{amb}}=0﹩, 1, 2, and 3 cm−3) computed by the MAIHEM hydrodynamic simulations with the cluster radius of R sc = 1 pc and the fixed cluster mass of 2.05 × 106 M ⊙. The current age of the hydrodynamic iteration is 1 Myr. The wind classification modes based on the temperature profile are presented, namely, the adiabatic wind (AW), adiabatic bubble (AB), adiabatic, pressure-confined (AP), catastrophic cooling (CC), catastrophic cooling bubble (CB), catastrophic cooling, pressure-confined (CP), no expanding wind (NW), and momentum-conserving (MC), while the wind modes of the optically thick models are denoted by the bold font.