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Cited article:

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Near-infrared photometry of the central stars of planetary nebulae with the VVVX survey

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Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-timescale Variables, and the Unusual Nucleus of WeSb 1*

Soumyadeep Bhattacharjee, S. R. Kulkarni, Albert K. H. Kong, M. S. Tam, Howard E. Bond, Kareem El-Badry, Ilaria Caiazzo, Nicholas Chornay, Matthew J. Graham, Antonio C. Rodriguez, Gregory R. Zeimann, Christoffer Fremling, Andrew J. Drake, Klaus Werner, Hector Rodriguez, Thomas A. Prince, Russ R. Laher, Tracy X. Chen and Reed Riddle
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Corrigendum: “Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-timescale Variables, and the Unusual Nucleus of WeSb 1” (2025, PASP, 137, 024201)

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Periodic Variability of the Central Stars of Planetary Nebulae Surveyed through the Zwicky Transient Facility

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The evolutionary route to form planetary nebulae with central neutron star–white dwarf binary systems

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Physical and Kinematical Characteristics of Wolf–Rayet Central Stars and their Host Planetary Nebulae

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The path from the Chinese and Japanese observations of supernova 1181 AD, to a Type Iax supernova, to the merger of CO and ONe white dwarfs

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When the Stars Align: A 5σ Concordance of Planetary Nebulae Major Axes in the Center of Our Galaxy

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New Close Binary Central Stars of Planetary Nebulae from Gaia DR3 Epoch Photometry

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Monthly Notices of the Royal Astronomical Society: Letters 516 (1) L61 (2022)
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Planetary Nebulae: Sources of Enlightenment

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Planetary nebulae with Wolf–Rayet-type central stars – IV. NGC 1501 and its mixing layer

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