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Evolution and Gas Dynamics of Planetary Nebulae
Published online by Cambridge University Press: 22 September 2016
Extract
Since the last IAU Symposium on Planetary Nebulae at Tatranska-Lomnica, a number of significant theoretical and observational advances have been made in the study of nebular dynamics. The following review emphasizes the evolution of nebulae after they have been ejected from the central star and have become optically thin to most radiation.
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- Session VI: Evolution and Morphology of Planetary Nebulae
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- Copyright © Reidel 1978
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