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Deuterated Molecules in Interstellar Clouds

Published online by Cambridge University Press:  04 August 2017

Alwyn Wootten
Alwyn Wootten*
Affiliation:
National Radio Astronomy Observatory, Charlottesville, Virginia 22903, United States of America

Abstract

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We show that deuteration in DCN and HDCO probably derives from CH2D+ in warm clouds, and that the levels of deuteration observed in those clouds require that radiative association play an important role in the chemistry of interstellar clouds.

Type
Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 120: Astrochemistry , 1987 , pp. 311 - 319
Copyright
Copyright © Reidel 1987 

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