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The Dynamical Gas Evolution of Low-and Intermediate-Mass Stars: PN Formation
Published online by Cambridge University Press: 26 May 2016
Abstract
Planetary nebula (PN) formation is intimately linked to stellar evolution. The stellar wind during the AGB and post-AGB stages depends on the progenitor mass and determines, together with the radiation field of the star, the structure and evolution of PNe. We summarize the results of the PhD thesis of E. Villaver, where we combined the results of stellar evolution with a numerical code to study the PN formation process.
- Type
- Part III: Planetary Nebulae in the Scheme of Stellar Evolution
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- Copyright © Astronomical Society of the Pacific 2003