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Hot Core Chemistry: Gas Phase Molecule Formation in situ

Published online by Cambridge University Press:  07 August 2017

S.B. Charnley  and
A.G.G.M. Tielens
S.B. Charnley
Affiliation:
Space Science Division, NASA Ames Research Center, California 94035.
A.G.G.M. Tielens
Affiliation:
Space Science Division, NASA Ames Research Center, California 94035.

Abstract

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The possibility that the observed abundances of several molecules in the Orion Hot Core are due to gas phase neutral chemistry has been examined.

Information

Type
Chemistry of Interface Regions
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 317 - 318
Copyright
Copyright © Kluwer 1992 

References

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