Planetary nebula progenitors that swallow binary systems
Noam Soker (Technion, Israel)

TL;DR
This paper proposes that irregular planetary nebulae can result from complex triple-stellar interactions involving tight binary systems within AGB stars, leading to diverse destruction and ejection processes that shape nebula morphology.
Contribution
It introduces a novel scenario where triple-stellar evolution explains the formation of irregular planetary nebulae, expanding understanding of their diverse morphologies.
Findings
Approximately 12.5% of non-spherical PNe may result from triple-stellar evolution.
Triple-stellar interactions can produce highly asymmetrical, 'messy' nebulae.
Multiple destruction pathways lead to varied nebula morphologies.
Abstract
I propose that some irregular `messy' planetary nebulae owe their morphologies to triple-stellar evolution where tight binary systems evolve inside and/or on the outskirts the envelope of asymptotic giant branch (AGB) stars. In some cases the tight binary system can survive, in other it is destroyed. The tight binary system might breakup with one star leaving the system. In an alternative evolution, one of the stars of the brook-up tight binary system falls toward the AGB envelope with low specific angular momentum, and drowns in the envelope. In a different type of destruction process the drag inside the AGB envelope causes the tight binary system to merge. This releases gravitational energy within the AGB envelope, leading to a very asymmetrical envelope ejection, with an irregular and `messy' planetary nebula as a descendant. The evolution of the triple-stellar system can be in a…
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