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Numerical Models of Dynamical and Spectral Evolution of Planetary Nebulae
Published online by Cambridge University Press: 18 September 2017
Extract
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.
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- Copyright © Reidel 1983