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Symposium Conclusions II

Published online by Cambridge University Press:  22 September 2016

George B. Field
George B. Field*
Affiliation:
Center for Astrophysics, Harvard College Observatory and Smithsonian Astrophysical Observatory

Extract

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Dr. Osterbrock has given a comprehensive summary of the Symposium. I will discuss a few topics which seemed particularly interesting to me as a non-specialist: dust, the fate of pre-planetary ejecta, and inhomogeneities. Let me begin by describing a simple model of the planetary nebula (PN) phenomenon, which is suggested by the discussions we have heard at this Symposium, and which provides the framework for my other comments.

Type
Session VIII: Planetary Nebulae and Their Influence on the Galaxy
Information
Symposium - International Astronomical Union , Volume 76: Planetary Nebulae , 1978 , pp. 367 - 373
Copyright
Copyright © Reidel 1978 

References

Anders, E. 1971, Ann. Rev. Astron. Astrophys. 9, 1.Google Scholar
Field, G.B. 1974, Ap. J. 187, 453.CrossRefGoogle Scholar
Hawkins, G.S. 1964, Ann. Rev. Astron. Astrophys. 2, 149.CrossRefGoogle Scholar
Mathis, J.S., Rumpl, W. and Nordsieck, K.H. 1977, Ap. J., in press.Google Scholar
Spitzer, L. Jr. 1977, Comments on Astrophysics and Space Physics, in press.Google Scholar
Woolf, N.J. 1973, Interstellar Dust and Related Topics, ed. Greenberg, J.M. and Van de Hulst, H.C. (Dordrecht-Holland: D. Reidel Publishing Co.), p. 485.Google Scholar