The dust envelope of IRC +10216.
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.
- Publication:
-
Circumstellar Matter
- Pub Date:
- 1987
- Bibcode:
- 1987IAUS..122..535R
- Keywords:
-
- Circumstellar Dust:Mira Stars;
- Circumstellar Dust:Radiative Transfer;
- Mira Stars:Circumstellar Dust;
- Radiative Transfer:Circumstellar Dust