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Molecules in Stellar Winds

Published online by Cambridge University Press:  07 August 2017

Alfred E. Glassgold
Alfred E. Glassgold*
Affiliation:
Department of Physics, New York University 2 Washington Place, New York, NY 10003, USA

Abstract

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High mass-loss molecular winds are characterstic of two important phases of stellar evolution, very young protostars and stars on the asymptotic branch. Novel chemical processes in these winds suggest a variety of new astronomical observations.

Type
Near Stellar Environments
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 379 - 386
Copyright
Copyright © Kluwer 1992 

References

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