MW angular momentum PDFs for its: thin and thick disks (left), combined stellar disk (center), and DM halo (right). The underlying PDFs in thin black are well approximated by normal distributions for the stellar components (thick blue, orange, and turquoise curves) and by log normal for the DM ones (thick black and gray curves). Solid or faint colors show the predictions for the contracted or uncontracted NFW mass model, respectively.