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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
Interstellar medium magnetic field in bow shock modelling
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
The physical and chemical structure of Sagittarius B2