Relations between the azimuthal AM of the dynamical disk components and the AM modulus of the DM halo for the galaxy sample in Paper II. Same details as in Fig. 1, but for all the dynamical disks combined (left) and the stellar halos (right). Left panels: each galaxy with a double disk is represented by a single point with abscissa J_z = J_z, thin + J_z, thick. The highlighted cyan points in all panels correspond to the best MW analog in the NIHAO sample, g8.26e11.