Shaping Proto–Planetary and Young Planetary Nebulae with Collimated Fast Winds
- 20 March 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 586 (1) , 319-337
- https://doi.org/10.1086/346265
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.Comment: 30 Pages, 18 figureKeywords
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This publication has 57 references indexed in Scilit:
- Shapes and Shaping of Planetary NebulaeAnnual Review of Astronomy and Astrophysics, 2002
- Magnetohydrodynamic Stellar and Disk Winds: Application to Planetary NebulaeThe Astrophysical Journal, 2001
- Collimation of Astrophysical Jets: The Proto–Planetary Nebula H[CLC]e[/CLC] [CSC]3-1475[/CSC]The Astrophysical Journal, 1997
- A numerical simulation of a variable velocity jetThe Astrophysical Journal, 1994
- Fast, low-ionization emission regions and other microstructures in planetary nebulaeThe Astrophysical Journal, 1993
- Formation of the circumstellar shell around SN 1987AThe Astrophysical Journal, 1993
- The structure and evolution of radiatively cooling jetsThe Astrophysical Journal, 1990
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- The evolution of planetary nebulae. II - Dynamical evolution of elliptical PNs and collimated outflowsThe Astronomical Journal, 1987
- Hydromagnetic flows from accretion discs and the production of radio jetsMonthly Notices of the Royal Astronomical Society, 1982