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The dust envelope of IRC +10216

Published online by Cambridge University Press:  04 August 2017

Stephen T. Ridgway ,
Kitt Peak ,
John J. Keady  and
Los Alamos
Stephen T. Ridgway
Affiliation:
National Observatory2 Tucson AZ, 85726
Kitt Peak
Affiliation:
National Observatory2 Tucson AZ, 85726
John J. Keady
Affiliation:
National Laboratory Los Alamos, NM 87545
Los Alamos
Affiliation:
National Laboratory Los Alamos, NM 87545

Abstract

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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 

References

Ready, J.J., Hall, D.N.B., and Ridgway, S.T. 1986, Ap. J., in press.Google Scholar
Ridgway, S.T., and Keady, J.J. 1981, Phil. Trans. Roy. Soc. Lond. A., 303, 497.Google Scholar
Ridgway, S.T., and Keady, J.J. 1986 (in preparation).Google Scholar