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Planetary Nebulae in the Scheme of Binary Evolution

Published online by Cambridge University Press:  26 May 2016

Noam Soker
Noam Soker*
Affiliation:
Dept. of Physics, University of Haifa-Oranim, Tivon 36006, Israel

Abstract

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In this review I present the binary model for the shaping of planetary nebulae (PNe) as I view it, in the context of historical evolution of other models for the shaping of PNe over more than 30 years. In describing the binary model, I concentrate on works published since the last IAU meeting on PNe. I think stellar companions are behind the shaping of bipolar PNe, i.e., having two lobes with an equatorial waist between them, and extreme elliptical PNe, e.g., having a dense equatorial ring, but no lobes. The question of whether a planet is required to spin the progenitor in order to form a moderate elliptical PN, or whether single stars can form moderate elliptical PNe, I consider to be an open question.

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. 223 - 230
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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