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Paper: 3D Hydrodynamical Simulations of PNe
Volume: 313, Asymmetrical Planetary Nebulae III
Page: 480
Authors: Wareing, C.J.; O'Brien, T.J.; Bryce, M.
Abstract: Simulations have been carried out using a newly developed parallel hydrodynamic code. Simple density profiles of an asymmetric ambient medium surrounding a source of a post-AGB like wind were considered. Future work will consider the shaping of planetary nebulae via binary interaction. Specifically MyCn18 and the ancient PN surrounding the classical nova GK Per will be investigated.
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