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Two-Dimensional Radiation-Hydrodynamics Calculations of the Formation of 0-B Associations in Dense Molecular Clouds
Published online by Cambridge University Press: 12 April 2016
Abstract
Two-dimensional calculations of ionization-shockwave propagation into a curved molecular cloud are presented. Density enhancement occurs due to the combined effects of cloud curvature and radiation flow. The star formation process is expected to be enhanced near the edges of irregularly shaped molecular clouds.
- Type
- I. ID, 2D, and 3D Collapse of Interstellar Clouds
- Information
- International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 275 - 282
- Copyright
- Copyright © Reidel 1980