Add to ORKGThe 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}, =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.Fil: Peri, Cintia Soledad. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Araudo, Anabella Teresa. Consejo Nacional de Inv...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow ...
We present a deep radio-polarimetric observation of the stellar bow shock EB27 associated with the m...
The bow shock produced by the high-mass runaway star BD +43° 3654 (Comerón & Pasquali 2007) has been...
We present a study of the radio emission from a massive runaway star. The star forms a bow shock tha...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detect...
The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by t...
Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
[Context] There is a population of runaway stars that move at extremely high speeds with respect to ...
Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to t...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow ...
We present a deep radio-polarimetric observation of the stellar bow shock EB27 associated with the m...
The bow shock produced by the high-mass runaway star BD +43° 3654 (Comerón & Pasquali 2007) has been...
We present a study of the radio emission from a massive runaway star. The star forms a bow shock tha...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
The latest survey of stellar bow shocks (Peri et al. 2012, A&A, 538, 108) lists 28 candidates detect...
The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by t...
Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
[Context] There is a population of runaway stars that move at extremely high speeds with respect to ...
Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to t...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow ...
We present a deep radio-polarimetric observation of the stellar bow shock EB27 associated with the m...