Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-27T02:53:09.162Z Has data issue: false hasContentIssue false
  • English
  • Français

Hydrodynamical interpretation of basic nebular structures

Published online by Cambridge University Press:  15 December 2006

M. Steffen  and
D. Schönberner
M. Steffen
Affiliation:
Astrophysikalisches Institut Potsdam, 14482 Potsdam, Germany email: msteffen@aip.de, deschoenberner@aip.de
D. Schönberner
Affiliation:
Astrophysikalisches Institut Potsdam, 14482 Potsdam, Germany email: msteffen@aip.de, deschoenberner@aip.de
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Based on existing hydrodynamical simulations, we review our present understanding of the formation and evolution of planetary nebulae (PNe) and discuss the relevant processes responsible for the development of the basic (1D) nebular structures.

Keywords

hydrodynamics - radiative transfer - stars: evolution - stars: mass loss - planetary nebulae: generalindividual (IC 418, NGC 6826, NGC 2438, Abell 39, NGC 7027, NGC 6543)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 285 - 292
Copyright
© 2006 International Astronomical Union