The Bipolar Engines of post-AGB stars: Transient Dynamos and Common Envelopes
J. Nordhaus (Univ. of Rochester), E. G. Blackman (Univ. of Rochester)

TL;DR
This paper investigates transient dynamo mechanisms in post-AGB stars, exploring how magnetic fields and binary interactions can drive asymmetries and outflows, with implications for planetary nebula formation.
Contribution
It introduces a model of a transient $-$ dynamo operating in AGB stars, including the effects of back-reaction and binary interactions, to explain asymmetries in post-AGB objects.
Findings
A robust dynamo can operate in common envelope scenarios with a binary companion.
Back-reaction effects are significant in sustaining the dynamo.
Energy and angular momentum transfer from a companion enhances magnetic activity.
Abstract
The physical mechanism(s) responsible for transitioning from a spherical Asymptotic Giant Branch (AGB) star to an asymmetric post-AGB (pAGB) object is poorly understood. In particular, excess momenta in the outflows of pAGB objects suggest that a binary may be required to supply an additional source of energy and angular momentum. The extraction of rotational energy from the engine is likely fundamental and may be facilitated if a dynamo is operating in the interior. In this regard, single star magnetic outflow models have been proposed as mechanisms for producing and shaping PNe, however these models neglect the back-reaction of the large-scale magnetic field on the flow. Here we present a transient dynamo operating in the envelope of an AGB star in (1) an isolated setting and (2) a common envelope in which the secondary is a low-mass companion in-spiraling in the AGB…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Astro and Planetary Science
