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Cited article:

Longitudinal drift of Tayler instability eigenmodes as a possible explanation for super-slowly rotating Ap stars

L. L. Kitchatinov, I. S. Potravnov, A. A. Nepomnyashchikh

A&A, 638 (2020) L9

Published online: 2020-06-17

DOI: https://doi.org/10.1051/0004-6361/202037862

This article has been cited by the following article(s):

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Tayler Instability of Magnetic Field as the Possible Reason for the Period Changes in Ap Star 56 Ari

I. S. Potravnov and L. L. Kitchatinov
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Secular stability of surface abundance structures in the rapidly rotating Ap star 56 Ari

I. Potravnov, N. Piskunov and T. Ryabchikova
Astronomy & Astrophysics 689 A111 (2024)
https://doi.org/10.1051/0004-6361/202451052

Magnetic field measurements of sharp-lined Ap stars

S P Järvinen, S Hubrig, R Jayaraman, I Ilyin and M Schöller
Monthly Notices of the Royal Astronomical Society 516 (2) 2629 (2022)
https://doi.org/10.1093/mnras/stac2381