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Dust Shell Models for Infrared Sources

Published online by Cambridge University Press:  25 April 2016

A. R. Hyland  and
R. A. Gingold
A. R. Hyland
Affiliation:
Mount Stromlo and Siding Spring Observatories The Australian National University
R. A. Gingold
Affiliation:
Mount Stromlo and Siding Spring Observatories The Australian National University
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Extract

Recent reviews have demonstrated that a wide ranging selection of objects emit a major proportion of their energy at wavelengths longer than 1 µm, including such intrinsically different objects as late type stars, Be stars, F supergiants and novae. In the majority of cases the infrared radiation has been interpreted in terms of thermal radiation from a circumstellar shell of solid ‘dust’ particles. Any attempt at a detailed comparison of theoretical energy distributions with observed infrared photometry encounters the problems of uncertainties in the absolute calibration, and limited accuracy of the observations.

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Contributions
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Publications of the Astronomical Society of Australia , Volume 2 , Issue 3 , October 1972 , pp. 155 - 157
Copyright
Copyright © Astronomical Society of Australia 1972

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References

1 Neugebauer, G., Becklin, E., and Hyland, A. R., Ann. Rev. Astron. and Ap. 9, 67 (1971).CrossRefGoogle Scholar
2 Hyland, A. R., Proc. A.S.A., 2, 14 (1971).Google Scholar
3 Low, F. J. and Smith, B. J., Nature, 212, 675 (1966).Google Scholar
4 Low, F. J., Johnson, H. L., Kleinmann, D. E., Latham, A. S. and Geisel, S. L., Ap. J., 160, 531 (1970).CrossRefGoogle Scholar
5 Hyland, A. R., Becklin, E. E., Frogel, J. A. and Neugebauer, G., Astron. and Ap., 16, 204 (1972).Google Scholar
6 Becklin, E. E., Frogel, J. A., Hyland, A. R., Kristian, J. and Neugebauer, G., Ap. J. (Utters), 158, L133 (1969)CrossRefGoogle Scholar
7 Toombs, R. I., Becklin, E. E., Frogel, J. A., Law, S. K., Porter, F. C. and Westphal, J. A., Ap. J. (Letters), 173, L71 (1972).CrossRefGoogle Scholar
8 Larson, R. B., MNRAS, 145, 297 (1969).CrossRefGoogle Scholar
9 Gillett, F. C, Hyland, A. R. and Stein, W. A., Ap. J. (Letters), 162, L21 (1970).CrossRefGoogle Scholar
10 Lee, T. A. and Feast, M. W., Ap. J. (Letters), 157, L173 (1969).CrossRefGoogle Scholar
11 Hyland, A. R., Becklin, E. E., Neugebauer, G., and Wallerstein, G., Ap. J., 158, 619 (1969).CrossRefGoogle Scholar
12 Herbig, G. H., Ap. J., 162, 557 (1970).CrossRefGoogle Scholar