MHD Models for PNe

Details MHD Models for PNe MHD Models for PNe

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000rmxac...9..210g&link_type=abstract

"Astrophysical Plasmas: Codes, Models, and Observations, Proceedings of the conference held in Mexico City, October 25-29, 1999,

Astronomy and Astrophysics

Astrophysics

Scientific paper

A self-consistent scenario to explain the morphology of planetary nebulae is presented. This scenario is consistent with the Galactic distribution of different nebular types. This work addresses several controversial features that appear in planetary nebulae, which are easily solved by the inclusion of MHD effects. These features include the presence of axisymmetric and collimated outflows with linearly increasing kinematics, and the existence of asymmetrical morphologies such as point-symmetric nebulae.

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