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Planetary Nebulae and Wolf-Rayet Nebulae

Published online by Cambridge University Press:  26 May 2016

Y. Grosdidier
Y. Grosdidier*
Affiliation:
Instituto de Astrofísica de Canarias, Calle Vía Láctea s/n, E-38200 La Laguna (Tenerife), Spain Observatoire Astronomique de Strasbourg, UMR 7550, 11 rue de l'Université, F-67000 Strasbourg, France

Abstract

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In the present paper I review some important facts regarding the similarities and differences between Galactic planetary nebulae and Galactic Wolf-Rayet (WR) nebulae within the scope of stellar mass-loss history and its subsequent impact on the nebular dynamics and morphology. The case of planetary nebulae with [WR] nuclei, which allows one to perform a more direct comparison with WR nebulae, is emphasized. In particular, I describe the apparently ubiquitous turbulent-like phenomena originating in [WR] stellar atmospheres and the surrounding nebulae, and discuss the possible impact of turbulence on planetary nebula studies.

Type
Part IV: Central Stars and their Atmospheres
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 193 - 200
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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