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The Nitrogen Chemistry in Interstellar Clouds
Published online by Cambridge University Press: 04 August 2017
Abstract
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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
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- Copyright
- Copyright © Reidel 1987
References
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