Visual Wide Binaries and the Structure of Planetary Nebulae

Abstract

In a recent work Ciardullo et al. (1999) list 19 planetary nebulae surveyed by the Hubble Space Telescope for the presence of resolved visual binary companions of their central stars. For ten planetary nebulae they argue for probable physical association of the resolved stars with the central stars, while for nine the association is less likely. Such stellar companions, at orbital separations of hundreds to thousands of astronomical units, will cause the structures of these planetary nebulae to possess a non-axisymmetrical signatures. By using images from the literature of these 19 planetary nebulae, I demonstrate that the structures of the planetary nebulae are compatible in most cases with Ciardullo et al.'s arguments for an association, or not, of the resolved stars with the planetary nebulae central stars. This shows that the departure, or not, of a planetary nebula from having pure axisymmetrical structure can be used to strengthen an argument for an association, or a non-association, of a putative wide companion with the stellar progenitor of the nebula.

17 pages + 1 table (postscript), uses aasms4.sty, AJ in press

References in corpus (2)

• A Hubble Space Telescope Survey for Resolved Companions of Planetary-Nebula Nuclei
• Jets, knots and tails in planetary nebulae: NGC 3918, K 1-2 and Wray 17-1

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• Departure from Axisymmetry in Planetary Nebulae
• Morphological and kinematic signatures of a binary central star in the planetary nebula Hu 2-1
• Classification of Planetary Nebulae by their Departure from Axisymmetry
• Knots in the outer shells of the planetary nebulae IC 2553 and NGC 5882
• Two's company, three's a crowd: SALT reveals the likely triple nature of the nucleus of the extreme abundance discrepancy factor planetary nebula Sp 3
• Interacting planetary nebulae III: Verification and galactic population based on the measurements of Gaia EDR3