No CrossRef data available.
Article contents
New dust features in oxygen-rich envelopes
Published online by Cambridge University Press: 25 May 2016
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.
We report on the discovery of new solid state emission features in the ISO-SWS spectra of evolved oxygen-rich stars. These features appear in cool dust shells and are probably due to crystalline forms of silicates, and crystalline water ice.
- Type
- Grains and Pahs
- Information
- Symposium - International Astronomical Union , Volume 178: Molecules in Astrophysics: Probes and Processes , 1997 , pp. 367 - 370
- Copyright
- Copyright © Kluwer 1997
References
Jäger, C., Mutschke, H., Begemann, B., Dorschner, J., Henning, Th.
1994, A&A
292, 641.Google Scholar
You have
Access