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Cited article:

Characterizing the dynamical magnetosphere of the extremely slowly rotating magnetic O9.7 V star HD 54879 using rotational modulation of the Hα profile

Manfred Küker, S. P. Järvinen, S. Hubrig, Ilya Ilyin and M. Schöller
Astronomische Nachrichten 345 (4) (2024)
https://doi.org/10.1002/asna.20230169

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

A massive helium star with a sufficiently strong magnetic field to form a magnetar

Tomer Shenar, Gregg A. Wade, Pablo Marchant, Stefano Bagnulo, Julia Bodensteiner, Dominic M. Bowman, Avishai Gilkis, Norbert Langer, André Nicolas-Chené, Lidia Oskinova, Timothy Van Reeth, Hugues Sana, Nicole St-Louis, Alexandre Soares de Oliveira, Helge Todt and Silvia Toonen
Science 381 (6659) 761 (2023)
https://doi.org/10.1126/science.ade3293

A closer look at the binary content of NGC 1850

S Saracino, S Kamann, N Bastian, M Gieles, T Shenar, N Reindl, J Müller-Horn, C Usher, S Dreizler and V Hénault-Brunet
Monthly Notices of the Royal Astronomical Society 526 (1) 299 (2023)
https://doi.org/10.1093/mnras/stad2706

Constraints on the multiplicity of the most massive stars known: R136 a1, a2, a3, and c

T. Shenar, H. Sana, P. A. Crowther, K. A. Bostroem, L. Mahy, F. Najarro, L. Oskinova and A. A. C. Sander
Astronomy & Astrophysics 679 A36 (2023)
https://doi.org/10.1051/0004-6361/202346930

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)
https://doi.org/10.1093/mnras/stab3720

Detecting the intrinsic X-ray emission from the O-type donor star and the residual accretion in a supergiant fast X-ray transient in its faintest state

L. Sidoli, K. Postnov, L. Oskinova, et al.
Astronomy & Astrophysics 654 A131 (2021)
https://doi.org/10.1051/0004-6361/202141378

Ultraviolet line profiles of slowly rotating massive star winds using the ‘analytic dynamical magnetosphere’ formalism

C Erba, A David-Uraz, V Petit, et al.
Monthly Notices of the Royal Astronomical Society 506 (4) 5373 (2021)
https://doi.org/10.1093/mnras/stab1853

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 Formation of a 70 M⊙ Black Hole at High Metallicity

K. Belczynski, R. Hirschi, E. A. Kaiser, Jifeng Liu, J. Casares, Youjun Lu, R. O’Shaughnessy, A. Heger, S. Justham and R. Soria
The Astrophysical Journal 890 (2) 113 (2020)
https://doi.org/10.3847/1538-4357/ab6d77

Variability of OB stars from TESS southern Sectors 1–13 and high-resolution IACOB and OWN spectroscopy

S. Burssens, S. Simón-Díaz, D. M. Bowman, et al.
Astronomy & Astrophysics 639 A81 (2020)
https://doi.org/10.1051/0004-6361/202037700

The stellar and wind parameters of six prototypical HMXBs and their evolutionary status

R. Hainich, L. M. Oskinova, J. M. Torrejón, et al.
Astronomy & Astrophysics 634 A49 (2020)
https://doi.org/10.1051/0004-6361/201935498

Analysis of the X-ray emission from OB stars III: low-resolution spectra of OB stars

Elizaveta Ryspaeva and Alexander Kholtygin
Research in Astronomy and Astrophysics 20 (7) 108 (2020)
https://doi.org/10.1088/1674-4527/20/7/108

Bow shocks, bow waves, and dust waves – I. Strong coupling limit

William J Henney and S J Arthur
Monthly Notices of the Royal Astronomical Society 486 (3) 3423 (2019)
https://doi.org/10.1093/mnras/stz1043

3D MHD simulations and synthetic radio emission from an oblique rotating magnetic massive star

S Daley-Yates, I R Stevens and A ud-Doula
Monthly Notices of the Royal Astronomical Society 489 (3) 3251 (2019)
https://doi.org/10.1093/mnras/stz1982

Extreme resonance line profile variations in the ultraviolet spectra of NGC 1624-2: probing the giant magnetosphere of the most strongly magnetized known O-type star

A David-Uraz, C Erba, V Petit, et al.
Monthly Notices of the Royal Astronomical Society 483 (2) 2814 (2019)
https://doi.org/10.1093/mnras/sty3227

Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur Revisited

Blagoy Rangelov, Thierry Montmerle, S. R. Federman, Patrick Boissé and Stefano Gabici
The Astrophysical Journal 885 (2) 105 (2019)
https://doi.org/10.3847/1538-4357/ab43e5

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

S Hubrig, M Küker, S P Järvinen, et al.
Monthly Notices of the Royal Astronomical Society 484 (4) 4495 (2019)
https://doi.org/10.1093/mnras/stz198

The shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system

T. Shenar, R. Hainich, H. Todt, et al.
Astronomy & Astrophysics 616 A103 (2018)
https://doi.org/10.1051/0004-6361/201833006