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Paper: The Hydro Models Session
Volume: 313, Asymmetrical Planetary Nebulae III
Page: 462
Authors: Lopez, J.A.
Abstract: Hydrodynamic models play a central role in our understanding of how planetary nebulae form and evolve. The hydro models session at this conference was particularly interesting for it included excellent talks ranging from the development of large scale structures in PNe, such as halos, to studies of collimated outflows and hypersonic bullets, the effects of stellar rotation on the nebular shell and warped toroids as a way to explain the origin of point-symmetry and poly-polarity. This diversity of topics exemplifies the current vigorous quest in the field for answers to topical problems in PN research. I present here a brief overview of these talks in the order they were scheduled during the conference.
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