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Dynamical Evolution of a Model Planetary Nebula

Published online by Cambridge University Press:  14 August 2015

W. G. Mathews
W. G. Mathews*
Affiliation:
University of California, San Diego, U.S.A.

Extract

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The gas-dynamical equations for conservation of mass, momentum and energy, the ionization equation, and the equation of transfer for the ionizing radiation have been solved in a manner which approximates conditions in planetary nebulae. The ionized and neutral gas are assumed to heat and cool according to a linearized rate proportional to

Type
Session IV – Structure and Dynamics
Information
Symposium - International Astronomical Union , Volume 34: Planetary Nebulae , 1968 , pp. 273 - 274
Copyright
Copyright © Reidel 1968 

References

Mathews, W.G. (1966) Astrophys. J., 143, 173.Google Scholar