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Paper: Magnetohydrodynamic Models for Planetary Nebulae
Volume: 199, Asymmetrical Planetary Nebulae II: From Origins to Microstructures
Page: 235
Authors: García-Segura, G.; Franco, J.; López, J. A.
Abstract: In this work, we address several controversial features that appear in Planetary Nebulae which are easily solved by the inclusion of magnetohydrodynamic effects. These features include the presence of axisymmetric flows, confinement of flows, linearly encreasing kinematics of collimated outflows and asymmetrical morphologies such as point- symmetric nebulae.
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