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Pre-planetary nebulae: a context for principles, progress, and questions on how binaries and magnetic fields produce jets

Published online by Cambridge University Press:  30 November 2022

Eric G. Blackman Open the ORCID record for Eric G. Blackman [Opens in a new window]
Eric G. Blackman*
Affiliation:
Department of Physics and Astronomy, University of RochesterRochester, NY, 14621, USA email: [email protected] Laboratory for Laser Energetics, University of RochesterRochester, NY, 14623, USA
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Abstract

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Astrophysical outflows treated initially as spherically symmetric often show evidence for asymmetry once seen at higher resolution. The preponderance of aspherical and multipolar planetary nebulae (PN) and pre-planetary nebulae (PPN) was evident after many observations from the Hubble Space Telescope. Binary interactions have long been thought to be essential for shaping asymmetric PN/PPN, but how? PPN are the more kinematically demanding of the two, and warrant particular focus. I address how progress from observation and theory suggests two broad classes of accretion driven PPN jets: one for wider binaries (PPN-W) where the companion is outside the outer radius of the giant and accretes via Roche lobe overflow, and the other which occurs in the later stages of CE for close binaries (PPN-C). The physics within these scenarios connects to progress and open questions about the role and origin of magnetic fields in the engines and in astrophysical jets more generally.

Keywords

(ISM:) planetary nebulae: generalISM: jets and outflowsstars: magnetic fieldsstars: windsoutflowsstars: AGB and post-AGB(stars:) binaries (including multiple): close
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S366: The Origin of Outflows in Evolved Stars , November 2020 , pp. 281 - 300
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Copyright
© The Author(s), 2022. Published by Cambridge University Press on behalf of International Astronomical Union

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