Recognition: unknown
Shaping Proto-Planetary and Young Planetary Nebulae with Collimated Fast Winds
classification
🌌 astro-ph
keywords
collimatednebulaefastplanetaryproto-planetaryshapingsimulationswind
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.