The environs of the massive runaway star BD+43 3654

The very massive runaway star BD+43° 3654 (O4 If) seems to be related with a bow shock detected by the MSX mission, that would be the result of the interaction of the strong stellar wind with the ambient matter. Shock-accelerated electrons will cool through synchrotron radiation producing a non-ther...

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Detalles Bibliográficos
Autores principales: Peri, Cintia Soledad, Benaglia, Paula, Romero, Gustavo Esteban, Martí, J.
Formato: Articulo Comunicacion
Lenguaje:Inglés
Publicado: 2010
Materias:
Astronomía
Interstellar medium
Jets
Outflows
Mass loss
HII regions
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/101969
https://ri.conicet.gov.ar/11336/6317
http://www.astroscu.unam.mx/rmaa/RMxAC..38/PDF/RMxAC..38_cperi.pdf
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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