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.
- Pub Date:
- Circumstellar Dust:Mira Stars;
- Circumstellar Dust:Radiative Transfer;
- Mira Stars:Circumstellar Dust;
- Radiative Transfer:Circumstellar Dust