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Dynamical PN Evolution with Magnetic Fields

Garcia-Segura
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Abstract

Hydrodynamical simulations played an important role in understanding the dynamics and shaping of planetary nebulae in the past century. However, hydrodynamical simulations were just a first order approach. The new millennium arrived with the generalized understanding that the effects of magnetic fields were necessary to study the dynamics of planetary nebulae. Thus, B-fields introduced a whole new number of physical possibilities for the modeling. In this paper, we review observational works done in the last 5 years and several works on magnetohydrodynamics about proto-planetary nebulae, since all the effort has been focused on that stage, and discuss different scenarios for the origin of magnetized winds, and the relation binary-bipolararity.

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Garcia-Segura. 2006-06-26. Dynamical PN Evolution with Magnetic Fields. https://doi.org/10.1017/s1743921306003127

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