Abstract
Introduction Nearby Molecular Clouds Molecular Cloud Constituents Cloud Diversity Density Probes Dense Cores Star Formation Elongation Virial Balance Ionization and Field-Neutral Coupling Line Width-Size Relations Associated Stars Core Size Temperature External Excitation of Core Turbulence Cluster-Forming Cores Models of Clustered Star Formation Observational Studies of Young Clusters Kernel Model Inward Motions in Dense Cores Infall Asymmetry Infall Asymmetry in Starless Cores Turbulent Cooling Flows Summary
Cite
CITATION STYLE
Myers, P. C. (1999). Physical Conditions in Nearby Molecular Clouds. In The Origin of Stars and Planetary Systems (pp. 67–96). Springer Netherlands. https://doi.org/10.1007/978-94-011-4509-1_3
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