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Temperature distributions in circumstellar dust shells
Published online by Cambridge University Press: 04 August 2017
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The knowledge of the temperature distribution in circumstellar dust shells (CDS) is needed for both the calculation of the emergent IR spectrum and the modelling of physical processes, e.g. dust formation.
- Type
- Circumstellar Dust and Chemistry
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 557 - 558
- Copyright
- Copyright © Reidel 1987
References
Gürtler, J., Henning, Th., Dorschner, J., and Friedemann, C.: 1985, Astron. Nachr.
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Henning, Th., Friedemann, C., Gürtler, J., and Dorschner, J.: 1984, Astron. Nachr.
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