Abstract
Magnetic Support of Clouds Fragmentation Empirical Measurements of the Mass-to-Flux Ration Turbulent Support of Molecular Clouds Filamentary Structure in Molecular Clouds Sustenance of Cloud Turbulence Through YSO Outflows A Toy Model of GMC Structure and Evolution Formation and Evolution of Molecular Cloud Cores The Pivotal State Self-Similar Collapse of Singular Isothermal Toroids Mass Loss from Stars and Disks Generalized X-wind Model Summary
Cite
CITATION STYLE
Shu, F. H., Allen, A., Shang, H., Ostriker, E. C., & Li, Z.-Y. (1999). Low-Mass Star Formation: Theory. In The Origin of Stars and Planetary Systems (pp. 193–226). Springer Netherlands. https://doi.org/10.1007/978-94-011-4509-1_6
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