Shaping Proto-Planetary and Young Planetary Nebulae with Collimated Fast Winds
Preprint
- 22 November 2002
Abstract
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.Keywords
All Related Versions
- Version 1, 2002-11-22, ArXiv
- Published version: The Astrophysical Journal, 586 (1), 319.
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