Dependence of Mg II absorption on different galaxy properties. From left to right and top to bottom: log(M^*), log(SFR), log(sSFR), redshift z, inclination i, azimuthal angle α, velocity dispersion at 2 R_d, circular velocity at 2 R_d, and v/σ at 2 R_d as a function of the impact parameter for the isolated galaxies. Galaxies associated with absorption with $W_{\mathrm{r}}^{2796}$ > 0.1 Å are represented by blue dots. Galaxies with no absorption detected, or absorptions with $W_{\mathrm{r}}^{2796}$ < 0.1 Å, are represented by gray crosses. For M_⋆, SFR, sSFR, and z, we show all 128 isolated galaxies (the 66 log(M_⋆/M_⊙) > 9 isolated galaxies are represented with big markers and the 62 log(M_⋆/M_⊙) < 9 isolated galaxies are represented by small ones). For inclination, velocity dispersion, circular velocity, and v/σ, we only show rotation-dominated isolated galaxies (55) and for α, those with i > 30° (46).