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Molecular catastrophes and the formation of circumstellar dust
Published online by Cambridge University Press: 04 August 2017
Abstract
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Radiative instabilities due to simple molecules may convert chromospheric material into masering molecules and dust capable of being removed from the star by radiation pressure.
- Type
- Circumstellar Dust and Chemistry
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 529 - 531
- Copyright
- Copyright © Reidel 1987
References
Clayton, D.
1985 in Interrelationships Among Circumstellar, Interstellar and Interplanetary Dust, NASA Conf. Publ. 2403.Google Scholar
Lane, A.
1984 in VLBI and Compact Radio Sources, eds. Fanti, et al. (Dordrecht; Reidel), p. 329.CrossRefGoogle Scholar
Lepp, S., McCray, R., Shull, J.M., Woods, T. and Kallman, T.
1985, Ap. J., 288, 58.CrossRefGoogle Scholar
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