The bow shock produced by the high-mass runaway star BD +43° 3654 (Comerón & Pasquali 2007) has been detected as a non-thermal radio source (S_ν ∝ ν^{-α}, <α>=0.5) and it is the first one of that type ever observed (Benaglia ...

The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detected at IR wavelengths, associated with massive, early-type stars up to 3 kpc, along with the geometrical parameters of the ...

We present a deep radio-polarimetric observation of the stellar bow shock EB27 associated with the massive star BD+43○3654. This is the only stellar bow shock confirmed to have non-thermal radio emission. We used the Jansky ...

Massive runaway stars produce bow shocks through the interaction of their winds with the interstellar medium, with the prospect for particle acceleration by the shocks. These objects are consequently candidates for non-thermal ...

Runaway masive stars are O- and B-type stars with large peculiar veloci- ties. Runaway OB stars can produce stellar bowshocks in the surrounding interstellar medium. Bowshocks develop as arc-shaped structures while the ...