Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps

Observations of the intracluster medium (ICM) in galaxy clusters suggest for the presence of turbulence and the magnetic fields' existence has been proved through observations of Faraday Rotation (FR) and synchrotron emission. The ICM is also known to be filled by a rarefied weakly collisional...

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Detalles Bibliográficos
Autores principales:	Nakwacki, M.S., Kowal, G., Santos-Lima, R., De Gouveia Dal Pino, E.M., Falceta-Gonçalves, D.A.
Formato:	JOUR
Materias:	Galaxies: clusters: intracluster medium Magnetic fields Methods: numerical Turbulence
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00358711_v455_n4_p3702_Nakwacki
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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