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Chemical Diagnostics of Turbulent Magnetic Boundary Layers
Published online by Cambridge University Press: 19 July 2016
Abstract
Results from models of the chemical evolution at the interfaces between hot, highly-ionized, stellar winds and cool, weakly-ionized, molecular clumps are presented.
- Type
- 6. Magnetic Fields in Molecular Clouds, Dark Globules and in the Pre-Stellar and Circumstellar Environment
- Information
- Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 349 - 350
- Copyright
- Copyright © Kluwer 1990