The Hydro Models Session

Details The Hydro Models Session The Hydro Models Session

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313..462l&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

Scientific paper

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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