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Numerical Models of Dynamical and Spectral Evolution of Planetary Nebulae

Published online by Cambridge University Press:  18 September 2017

V. A. Okorokov ,
B. M. Shustov ,
A. V. Tutukov  and
H. W. Yorke
V. A. Okorokov
Affiliation:
Astronomical Council of the USSR Academy of Sciences, Moscow, USSR
B. M. Shustov
Affiliation:
Astronomical Council of the USSR Academy of Sciences, Moscow, USSR
A. V. Tutukov
Affiliation:
Astronomical Council of the USSR Academy of Sciences, Moscow, USSR
H. W. Yorke
Affiliation:
Universitäts-Sternwarte, Göttingen, W. Germany

Extract

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Numerical models of planetary nebulae (PN) dynamical evolution are calculated under the assumption of spherical symmetry and discussed in the light of infrared, radio and optical observations. The set of hydrodynamical equations is solved simultaneously with equations for nongrey radiative transfer.

Type
Abstracts of Contributed Papers
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 317 - 318
Copyright
Copyright © Reidel 1983