Magnetopause distance as a function of the stellar radius of representative stars from our sample. The blue and orange lines represent Case 1 (only stellar magnetic pressure is considered) and Case 3 (stellar magnetic and ram pressures are considered) with slow wind, respectively. The red line is Case 1 with the alternative magnetic field decay B_r ∝ r^−5/3. The solid green area is the HZ of the star. The gray horizontal dashed lines indicate the size of the magnetosphere of early (5r_p) and modern Earth (11.7r_p). The black vertical dotted lines represent the different tidal locking regimes assuming Q = 100 (see Section 3.2).