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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

Eva Villaver ,
Arturo Manchado  and
Guillermo García-Segura
Eva Villaver
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
Arturo Manchado
Affiliation:
Instituto de Astrofísica de Canarias, c/ Via Láctea s/n 38205 La Laguna (Tenerife), Spain
Guillermo García-Segura
Affiliation:
Instituto de Astronomía-Universidad Nacional Autónoma de México, Apartado Postal 877, Ensenada, 22830 Baja California, México

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 155 - 156
Copyright
Copyright © Astronomical Society of the Pacific 2003