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Chemical Diagnostics of Turbulent Magnetic Boundary Layers

Published online by Cambridge University Press:  19 July 2016

S. B. Charnley
S. B. Charnley*
Affiliation:
Max-Planck-Institut für Physik und Astrophysik Institut für extraterrestrische Physik D-8046 Garching bei München, Federal Republic of Germany

Abstract

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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 

References

1. Hartquist, T.W. and Dyson, J.E. (1988), Astrophys. Space. Sci. , 144, 615.Google Scholar
2. Goldsmith, P.F., Langer, W.D. and Wilson, R.W. (1986), Ap.J. (Letters) , 303, L11.CrossRefGoogle Scholar
3. Charnley, S.B., Dyson, J.E., Hartquist, T.W. and Williams, D.A. (1988), Mon. Not. R. astr. Soc. , 235, 1257.Google Scholar
4. Charnley, S.B., Dyson, J.E., Hartquist, T.W. and Williams, D.A. (1989), Mon. Not. R. astr. Soc. , submitted.Google Scholar