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The Nitrogen Chemistry in Interstellar Clouds
Published online by Cambridge University Press: 04 August 2017
Abstract
Our time dependent model of chemistry of dense interstellar clouds has been extended to study the formation of nitrogen bearing molecules. Here we present results for the calculations, under a variety of density, temperature, and elemental conditions, of the abundances of the following observationally important species: CN, HCN, HNC, NH3, NO, and N2H.
- Type
- Interstellar Medium
- Information
- Copyright
- Copyright © Reidel 1987