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The Optical Properties of Circumstellar and Interstellar Dust in the Mid-IR
Published online by Cambridge University Press: 12 April 2016
Abstract
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We deduce the optical efficiency Q (λ)/ a of the circumstellar dust material over the range 8-30 μm from twelve M and G giants and supergiants and that of the dust present in the general ISM and molecular clouds from thirteen protostars. We then discuss the differences between these two profiles in the light of the condensation theory.
- Type
- IV. Optical Studies of Dust
- Information
- International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 267 - 271
- Copyright
- Copyright © Reidel 1985
References
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