High resolution version of The first stars: formation of binaries and small multiple systems The following are movies of the simulation presented in the paper. Watch them to view the formation of a small multiple system of Pop III stars from a disk of primordial gas. Density in x-y plane Density in x-z plane Temperature in x-y plane Temperature in x-z plane The following shows the evolution of the entire 140 kpc (comoving) cosmological box. Also shown is the central 20 kpc (comoving), in which we can see the assembly of the minihalo hosting the Pop III stars. full cosmological box (140 kpc) central 20 kpc Below is the corresponding DM distribution on various scales at z = 23.75 in the simulation. Click to see the enlarged image.