Why Magnetic Fields Cannot Be the Main Agent Shaping Planetary Nebulae

@article{Soker2006WhyMF,
  title={Why Magnetic Fields Cannot Be the Main Agent Shaping Planetary Nebulae},
  author={Noam Soker},
  journal={Publications of the Astronomical Society of the Pacific},
  year={2006},
  volume={118},
  pages={260 - 269}
}
  • N. Soker
  • Published 28 January 2005
  • Physics
  • Publications of the Astronomical Society of the Pacific
An increasing amount of the literature reports the detection of magnetic fields in asymptotic giant branch (AGB) stars and in central stars of planetary nebulae (PNe). These detections lead to claims that the magnetic fields are the main agent shaping the PNe. In this paper, I examine the energy and angular momentum carried by magnetic fields expelled from AGB stars, as well as other physical phenomena that accompany the presence of large‐scale fields, such as those claimed in the literature. I… 
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  • E. Blackman
  • Physics
    Proceedings of the International Astronomical Union
  • 2008
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Isolated versus common envelope dynamos in planetary nebula progenitors
The origin, evolution and role of magnetic fields in the production and shaping of protoplanetary nebulae (PPNe) and planetary nebulae (PNe) are a subject of active research. Most PNe and PPNe are
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TLDR
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