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Progress in Interstellar Molecule Formation

  • William D. Watson
Part of the Astrophysics and Space Science Library book series (ASSL, volume 70)

Abstract

Selected observational, laboratory and theoretical results from the past few years which are significant for delineating interstellar molecule reactions are presented. Molecular species for which reaction mechanisms are considered include OH, NH, CH, and CH+ in diffuse interstellar clouds, and HCO+, N2H+, HCN, HNC, and H2CO in dense clouds.

Keywords

Rate Coefficient Dense Cloud Interstellar Cloud Strong Emission Line Diffuse Cloud 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1977

Authors and Affiliations

  • William D. Watson
    • 1
  1. 1.Departments of Physics and AstronomyUniversity of IllinoisUSA

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