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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 The Astrophysical Journal 977(1) 84 (2024) https://doi.org/10.3847/1538-4357/ad865a
On the plerionic rectangular supernova remnants of static progenitors
D M-A Meyer, Z Meliani, P F Velázquez, M Pohl and D F Torres Monthly Notices of the Royal Astronomical Society 527(3) 5514 (2023) https://doi.org/10.1093/mnras/stad3495
Detection of anomalous element distribution in the extremely slowly rotating magnetic O9.7 V star HD 54879
Testing the fossil field hypothesis: could strongly magnetized OB stars produce all known magnetars?
Ekaterina I Makarenko, Andrei P Igoshev and A F Kholtygin Monthly Notices of the Royal Astronomical Society 504(4) 5813 (2021) https://doi.org/10.1093/mnras/stab1175
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 Monthly Notices of the Royal Astronomical Society: Letters 492(1) L1 (2020) https://doi.org/10.1093/mnrasl/slz174
The very slow rotation of the magnetic O9.7 V star HD 54879
S Hubrig, S P Järvinen, M Schöller and C A Hummel Monthly Notices of the Royal Astronomical Society 491(1) 281 (2020) https://doi.org/10.1093/mnras/stz3046
The Origin of the Bimodal Distribution of Magnetic Fields in Early-type Stars