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...
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| Autores principales: | , , , , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
2011
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| 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: |
| id |
I19-R120-10915-100791 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas Stars: mass loss |
| spellingShingle |
Ciencias Astronómicas Stars: mass loss Peri, Cintia Soledad Araudo, Anabella Teresa Benaglia, Paula Romero, Gustavo Esteban Martí, Josep Analysis of the spectral energy distribution from a runaway star bow shock |
| topic_facet |
Ciencias Astronómicas Stars: mass loss |
| description |
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. |
| format |
Articulo Comunicacion |
| author |
Peri, Cintia Soledad Araudo, Anabella Teresa Benaglia, Paula Romero, Gustavo Esteban Martí, Josep |
| author_facet |
Peri, Cintia Soledad Araudo, Anabella Teresa Benaglia, Paula Romero, Gustavo Esteban Martí, Josep |
| author_sort |
Peri, Cintia Soledad |
| title |
Analysis of the spectral energy distribution from a runaway star bow shock |
| title_short |
Analysis of the spectral energy distribution from a runaway star bow shock |
| title_full |
Analysis of the spectral energy distribution from a runaway star bow shock |
| title_fullStr |
Analysis of the spectral energy distribution from a runaway star bow shock |
| title_full_unstemmed |
Analysis of the spectral energy distribution from a runaway star bow shock |
| title_sort |
analysis of the spectral energy distribution from a runaway star bow shock |
| publishDate |
2011 |
| url |
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 |
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AT pericintiasoledad analysisofthespectralenergydistributionfromarunawaystarbowshock AT araudoanabellateresa analysisofthespectralenergydistributionfromarunawaystarbowshock AT benagliapaula analysisofthespectralenergydistributionfromarunawaystarbowshock AT romerogustavoesteban analysisofthespectralenergydistributionfromarunawaystarbowshock AT martijosep analysisofthespectralenergydistributionfromarunawaystarbowshock |
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Repositorios |
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