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Cited article:

The arc-shaped radio source at the centre of NGC 6334A: is it a colliding wind region of two young massive stars or the bow shock of a runaway star?

Vanessa Yanza, Sergio A Dzib, Aina Palau, Luis F Rodríguez, Josep M Masqué, Pedro R Rivera-Ortiz and Sac-Nicté X Medina
Monthly Notices of the Royal Astronomical Society 538 (3) 1314 (2025)
https://doi.org/10.1093/mnras/staf344

Particle acceleration at the bow shock of runaway star LS 2355: non-thermal radio emission but no γ-ray counterpart

J van den Eijnden, S Mohamed, F Carotenuto, S Motta, P Saikia and D R A Williams-Baldwin
Monthly Notices of the Royal Astronomical Society 532 (3) 2920 (2024)
https://doi.org/10.1093/mnras/stae1622

Search for particle acceleration in two massive Wolf–Rayet stars using uGMRT observations

Anindya Saha, Anandmayee Tej, Santiago del Palacio, Michaël De Becker, Paula Benaglia, C H Ishwara-Chandra and Prachi Prajapati
Monthly Notices of the Royal Astronomical Society 526 (1) 750 (2023)
https://doi.org/10.1093/mnras/stad2758