3D Hydrodynamical Simulations of PNe

Details 3D Hydrodynamical Simulations of PNe 3D Hydrodynamical Simulations of PNe

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313..480w&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

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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