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Dust in Planetary Nebulae
Published online by Cambridge University Press: 22 September 2016
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In this review I shall concentrate on theoretical aspects of dust in planetary nebulae (PN), since Dr. Balick has reviewed observations in the preceding paper. I shall consider the questions, how much dust is there in PN? What is its composition? What effects does it have on the ionization structure? On the dynamics of the nebula?
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- Session VI: Evolution and Morphology of Planetary Nebulae
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- Copyright © Reidel 1978
References
Becklin, E. E., Neugebauer, G., and Wynn-Williams, C. G.: 1973, Astrophys. Letters
15, 87.Google Scholar
Hicks, T. R., Phillips, J. P., and Reay, N. K.: 1976, Monthly Notices Roy. Astron. Soc.
176, 409.Google Scholar
Klucker, R., Skibowski, M., and Steinman, W.: 1974, Physica status solidi (b)
65, 703.CrossRefGoogle Scholar
MacGregor, A. D., Magro, C. S., Selby, M. J., and Whiteoak, P. A.: 1976, Astron. Astrophys.
50, 389.Google Scholar
Panagia, N.: 1976, in “Infrared and Submillimeter Astronomy”
Fazio, G. G. (ed.), D. Reidel Publishing Co., Dordrecht, Holland, p. 43.Google Scholar
Panagia, N., Bussoletti, E., and Blanco, A.: 1977, in “CNO Isotopes in Astrophysics”, Audouze, J. (ed.), D. Reidel Publishing Co., Dordrecht, Holland, p. 45.CrossRefGoogle Scholar
Pottasch, S., Wesselius, P., Wu, C.-C., and van Duinen, R. J.: 1977, Astron. Astrophys.
54, 435.Google Scholar
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