Kohoutek 1-9's central star is a dwarf barium star with the nebula showing a thin-ring morphology consistent with binary ejection in the orbital plane.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
years
2026 2representative citing papers
Morphological similarity between pipe features in PNe and CCSNRs and a jet simulation is used to argue that jets formed the pipes and to bolster the JJEM for core-collapse supernovae.
citing papers explorer
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Spectroscopic Survey of Faint Planetary-Nebula Nuclei. VIII. The Dwarf Barium Central Star of Kohoutek 1-9
Kohoutek 1-9's central star is a dwarf barium star with the nebula showing a thin-ring morphology consistent with binary ejection in the orbital plane.
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The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants
Morphological similarity between pipe features in PNe and CCSNRs and a jet simulation is used to argue that jets formed the pipes and to bolster the JJEM for core-collapse supernovae.