The Structuring of Planetary Nebulae

Details The Structuring of Planetary Nebulae The Structuring of Planetary Nebulae

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..784..226g&link_type=abstract

MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures. AIP Conference Proceedings, Volume 784, pp

Physics

Planetary Nebulae, Magnetohydrodynamics, Interstellar Matter, Giant Stars, Physical Properties, Planetary Nebulae, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

This paper discusses some features in Planetary Nebulae and Protoplanetary Nebulae that are addressed by several works on MHD. We review different scenarios for the origin of magnetized winds, either for Protoplanetary Nebulae or Planetary Nebulae, and discusses the production of axisymmetric flows, the confinement of flows and the production of jets and ansae, point-symmetric nebulae and the periodic shells around Planetary Nebulae and Protoplanetary Nebulae.

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