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Cited article:

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First Observation of the Complete Rotation Period of the Ultraslowly Rotating Magnetic O Star HD 54879

C. Erba, C. P. Folsom, A. David-Uraz, G. A. Wade, S. Seadrow, S. Bellotti, L. Fossati, V. Petit and M. E. Shultz
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On the plerionic rectangular supernova remnants of static progenitors

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Detection of anomalous element distribution in the extremely slowly rotating magnetic O9.7 V star HD 54879

S P Järvinen, S Hubrig, M Schöller, et al.
Monthly Notices of the Royal Astronomical Society 510 (3) 4405 (2022)
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On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars

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The Astrophysical Journal 915 (2) 112 (2021)
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Testing the fossil field hypothesis: could strongly magnetized OB stars produce all known magnetars?

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Monthly Notices of the Royal Astronomical Society 504 (4) 5813 (2021)
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No evidence of a sudden change of spectral appearance or magnetic field strength of the O9.7V star HD 54879

G A Wade, S Bagnulo, Z Keszthelyi, C P Folsom, E Alecian, N Castro, A David-Uraz, L Fossati, V Petit, M E Shultz and J Sikora
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The very slow rotation of the magnetic O9.7 V star HD 54879

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The Origin of the Bimodal Distribution of Magnetic Fields in Early-type Stars

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A short and sudden increase of the magnetic field strength and the accompanying spectral variability in the O9.7 V star HD 54879

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Monthly Notices of the Royal Astronomical Society 484 (4) 4495 (2019)
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The MiMeS survey of magnetism in massive stars: magnetic properties of the O-type star population

V Petit, G A Wade, F R N Schneider, et al.
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