No CrossRef data available.
Article contents
Molecular Formation in Hot Diffuse Clouds
Published online by Cambridge University Press: 14 August 2015
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
A description is given of the processes of molecular formation and destruction in diffuse interstellar clouds and detailed models of the clouds lying towards ζ Ophiuchi, ζ Persei and o Persei are used to assess the validity of gas phase chemistry. Modifications that may arise from shock-heated regions are discussed.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 273 - 280
- Copyright
- Copyright © Reidel 1980
References
Chaffee, F.H., Lutz, B.L., Black, J.H., Vanden Bout, P.A., and Snell, R.L.
1979, Ap. J. (Letters)
in press.Google Scholar
Chambaud, G., Launay, J.M., Levy, B., Millie, P., Roueff, E. and Tran Minh, F.
1979, this volume.Google Scholar
Dalgarno, A., de Jong, T., Oppenheimer, M. and Black, J.H.
1974, Ap. J. (Letters)
192, L37.Google Scholar
Hartquist, T.W., Black, J.H. and Dalgarno, A.
1978, Mon. Not. Roy. Astr. Soc.
185, 643.Google Scholar
You have
Access