Analysis of the spectral energy distribution from a runaway star bow shock
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<sub>ν</sub> ∝ ν<sup>-α</sup>, <α>=0.5) and it is the first one of that type ever observed (Benaglia et al. 2010). The non-t...
Guardado en:
| Autores principales: | , , , , |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
2011
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/100791 https://ri.conicet.gov.ar/11336/5209 http://www.astroscu.unam.mx/rmaa/RMxAC..40/PDF/RMxAC..40_cperi.pdf http://www.redalyc.org/articulo.oa?id=57121297079 |
| Aporte de: |
| Sumario: | 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<sub>ν</sub> ∝ ν<sup>-α</sup>, <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. |
|---|