Two-dimensional radiation-hydrodynamics calculations of the formation of O-B association in dense molecular clouds

Two-dimensional radiation-hydrodynamics calculations of the formation of O-B association in dense molecular clouds [electronic resource]

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 molec...

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Bibliographic Details
Online Access: Online Access
Corporate Author: University of California, Berkeley (Researcher)
Format: Government Document Electronic eBook
Language:English
Published: Berkeley, Calif. : Oak Ridge, Tenn. : University of California, Berkeley ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, 1980.
Subjects:
Cosmic Gases.
Shock Waves.
Hydrodynamic Model.
Molecules.
Star Accretion.
Two-Dimensional Calculations.
Wave Propagation.
Fluids.
Gases.
Mathematical Models.
Particle Models.
Star Evolution.
Statistical Models.
Thermodynamic Model.
Classical And Quantum Mechanics, General Physics.

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Call Number: E 1.99: conf-800872-8
E 1.99: conf-800872-8 Available

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