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Structure and Evolution of Planetary Nebula Haloes

Published online by Cambridge University Press:  26 May 2016

Matthias Steffen  and
Detlef Schönberner
Matthias Steffen
Affiliation:
Astrophysikalisches Institut Potsdam, Germany
Detlef Schönberner
Affiliation:
Astrophysikalisches Institut Potsdam, Germany

Abstract

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The density structure of the extended haloes of Planetary Nebulae (PN) is generally believed to reflect the previous history of heavy mass loss during the final stages of stellar evolution on the asymptotic giant-branch (AGB). In this review, we discuss different interpretations of the observed PN halo structures in the light of recent numerical simulations combining detailed AGB and post-AGB stellar evolution calculations with time-dependent hydrodynamical wind models.

Type
Part VII: Nebular Morphology and Dynamics
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 439 - 446
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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