Synchrotron radiation and absence of linear polarization in the colliding wind binary WR 146

Context. Several massive early-type binaries exhibit non-thermal emission which has been attributed to synchrotron radiation from particles accelerated by diffusive shock acceleration (DSA) in the wind-collision region (WCR). If the magnetic field in the strong shocks is ordered, its component paral...

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Detalles Bibliográficos
Autores principales: Hales, C. A., Benaglia, Paula, Palacio, Santiago del, Romero, Gustavo Esteban, Koribalski, B. S.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2017
Materias:
Ciencias Astronómicas
Polarization
Radiation mechanisms: non-thermal
Radio continuum: stars
Stars: individual: WR 146
Stars: winds, outflows
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/87671
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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