Non-thermal radiation from a runaway massive star

We present a study of the radio emission from a massive runaway star. The star forms a bow shock that is clearly observed in the infrared. We have performed VLA observations under the assumption that the reverse shock in the stellar wind might accelerate charged particles up to relativistic energies...

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Detalles Bibliográficos
Autores principales:	Romero, Gustavo Esteban, Benaglia, Paula, Peri, Cintia Soledad, Martí, Josep, Araudo, Anabella Teresa
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2011
Materias:	Ciencias Astronómicas Early-type stars Cherenkov telescope array
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/99537 https://ri.conicet.gov.ar/11336/5210 http://arxiv.org/abs/1011.2773v1
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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