2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/13741Giant molecular clouds (GMCs) are the sites of star formation in the Galaxy. Many of their properties can be understood in terms of a model in which the GMCs and the star-forming clumps within them are in approximate pressure equilibrium, with turbulent motions treated as a separate pressure component.38 pages. Conference: The Physics of Star Formation and Early Stellar Evolution (Crete II)Astrophysicstext