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Cited article:

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

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