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astro-ph.SR2026
Is the nitrogen-rich source PN K4-47 a true planetary nebula?
Thomas Steinmetz, Tomasz Kaminski, David Jones +3
PN K4-47 is a young planetary nebula that exhibits shock-excited bipolar lobes and a complex molecular environment, with the highest number of molecules detected within a planetary…
astro-ph.SR2024★ 1 cited
Low velocity streams inside the planetary nebula H 2-18. A 3D photoionization and kinematical reconstruction
K. Gesicki, A. Zijlstra, M. Hajduk +4
Aims. Numerous planetary nebulae show complicated inner structures not obviously explained. For one such object we undertake a detailed 3D photoionization and kinematical model ana…
astro-ph.SR2023
Binary central stars of planetary nebulae in the Large Magellanic Cloud
M. Gładkowski, M. Hajduk, R. Smolec +2
Close binary central stars of planetary nebulae (PNe) must have formed through a common envelope evolution during the giant phase experienced by one of the stars. Transfer of the a…