New results on planetary nebula shaping and stellar binarity
arXiv:1010.3802
Abstract
The question of what physical mechanisms shape planetary nebulae into their observed morphologies remains open. However, intensified efforts since the last meeting in this series, Asymmetrical Planetary Nebulae IV, in July 2007 have yielded some excellent results. In this review we concentrate on those developments that have taken place in the last three years, with emphasis on results obtained since the review by De Marco (2009).
9 pages, one figure, Proceedings of the Asymmetrical Planetary Nebula V conference (Lake District, June 2010. Invited Review)