2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/178337The interstellar medium (ISM) provides a unique laboratory for highly supersonic, driven hydrodynamics turbulence. We present a theory of such turbulence, confirm it by numerical simulations, and use the results to explain observational properties of interstellar molecular clouds, the regions where stars are born.5 pages, 3 figures includedAstrophysicsChaotic DynamicsFluid Dynamicstext