A Magnetohydrodynamic Model for the AGB Star: Preplanetary Nebula Symbiosis

Details A Magnetohydrodynamic Model for the AGB Star: Preplanetary Nebula Symbiosis A Magnetohydrodynamic Model for the AGB Star: Preplanetary Nebula Symbiosis

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pasp..122.1334p&link_type=abstract

Publications of the Astronomical Society of the Pacific, Volume 122, issue 897, pp.1334-1340

Astronomy and Astrophysics

Astronomy

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Ism

Scientific paper

In this article, a magnetohydrodynamic (MHD) model is presented that is aimed at understanding the anisotropic mass loss by an AGB star and subsequent bipolar planetary nebula formation. The main challenge in developing such a model was to simultaneously treat the dynamo engine in the core region of the AGB progenitor, magnetic buoyancy, meridional circulation, and gas ejection in a self-consistent manner. A previous article did not incorporate the dynamo and the feedback of the produced magnetic field on differential rotation.

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