Shaping Proto-Planetary and Young Planetary Nebulae with Collimated Fast Winds

Details Shaping Proto-Planetary and Young Planetary Nebulae with Collimated Fast Winds Shaping Proto-Planetary and Young Planetary Nebulae with Collimated Fast Winds

2002-11-22

arxiv.org/abs/astro-ph/0211510v1

Astrophys.J. 586 (2003) 319-337

Astronomy and Astrophysics

Astrophysics

30 Pages, 18 figures

Scientific paper

10.1086/346265

Using two-dimensional hydrodynamical simulations, we investigate the interaction of a collimated fast wind (CFW) interacting with a spherical asymptotic giant branch (AGB) wind as the mechanism for shaping proto-planetary nebulae and young planetary nebulae. In particular, we compare our simulations to the observations of an evolved PPN with multiple, highly collimated lobes, CRL 618.

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