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The dust envelope of IRC +10216
Published online by Cambridge University Press: 04 August 2017
Abstract
Infrared speckle measurements and photometry are used to assess the shape and thickness of the dust shell of the carbon rich Mira variable IRC + 10216. A spherically symmetric radiative transfer model has been developed to approximate the physical parameters.
- Type
- Circumstellar Dust and Chemistry
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 535 - 536
- Copyright
- Copyright © Reidel 1987