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Analysis of the spectral energy distribution from a runaway star bow shock / C. S. Peri ... [et al.].
— (Trabajos publicados del IAR ; no. 1132)
Revista mexicana de astronomía y astrofísica. Serie de conferencias — Universidad Autónoma de México. Instituto de Astronomía — Vol. 40, (2011), p. 156
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[elevado a la]{-α}, <α>=0.5) and it is the first one of that type ever observed (Benaglia et al. 2010). The non-thermal detection provides evidence of the presence of a magnetic field and relativistic electrons. This population of relativistic particles can produce high-energy (HE) emission
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