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Cited article:

Standing torsional Alfvén waves as the source of the rotational period variation in magnetic early-type stars

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New ACV variables discovered in the Zwicky Transient Facility survey

B. Bauer-Fasching, K. Bernhard, E. Brändli, H. Burger, B. Eisele, S. Hümmerich, J. Neuhold, E. Paunzen, M. Piecka, S. Ratzenböck and M. Prišegen
Astronomy & Astrophysics 687 A211 (2024)
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HD 34736: an intensely magnetised double-lined spectroscopic binary with rapidly rotating chemically peculiar B-type components

E Semenko, O Kochukhov, Z Mikulášek, G A Wade, E Alecian, D Bohlender, B Das, D L Feliz, J Janík, J Kolář, J Krtička, D O Kudryavtsev, J M Labadie-Bartz, D Mkrtichian, D Monin, V Petit, I I Romanyuk, M E Shultz, D Shulyak, R J Siverd, A Tkachenko, I A Yakunin and M Zejda
Monthly Notices of the Royal Astronomical Society 535 (3) 2812 (2024)
https://doi.org/10.1093/mnras/stae2503

A new sample of super-slowly rotating Ap (ssrAp) stars from the Zwicky Transient Facility survey

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Astronomy & Astrophysics 692 A231 (2024)
https://doi.org/10.1051/0004-6361/202452075

Magnetic Fields in Chemically Peculiar and Related Stars. IX. Main Results Obtained in 2022 and an Analysis of Immediate Prospects

I. I. Romanyuk
Astrophysical Bulletin 78 (4) 594 (2023)
https://doi.org/10.1134/S1990341323700244