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. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Araudo, Anabel...
Starburst galaxies generate large-scale winds powered by the activity in the star-forming regions lo...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Massive runaway stars produce bow shocks through the interaction of their winds with the interstella...
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...
[Context] There is a population of runaway stars that move at extremely high speeds with respect to ...
Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non...
The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by t...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow ...
Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to t...
Starburst galaxies generate large-scale winds powered by the activity in the star-forming regions lo...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Massive runaway stars produce bow shocks through the interaction of their winds with the interstella...
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...
[Context] There is a population of runaway stars that move at extremely high speeds with respect to ...
Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non...
The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by t...
Context. The environs of massive, early-type stars have been inspected in recent years in the search...
Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow ...
Context. Runaway massive stars are O-and B-type stars with high spatial velocities with respect to t...
Starburst galaxies generate large-scale winds powered by the activity in the star-forming regions lo...
Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic vel...
Massive runaway stars produce bow shocks through the interaction of their winds with the interstella...