The Dynamical Structure and Evolution of Giant Molecular Clouds
arXiv:astro-ph/9901370
Abstract
Giant 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)