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: Peri, Cintia Soledad, Araudo, Anabella Teresa, Benaglia, Paula, Romero, Gustavo Esteban, Martí, Josep
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:
id I19-R120-10915-100791
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 romerogustavoesteban analysisofthespectralenergydistributionfromarunawaystarbowshock
AT martijosep analysisofthespectralenergydistributionfromarunawaystarbowshock
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