Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps - II. The effects of instabilities feedback

Statistical analysis of Faraday rotation measure (RM) maps of the intracluster medium (ICM) of galaxy clusters provides a unique tool to evaluate some spatial features of the magnetic fields there. Its combination with numerical simulations of magnetohydrodynamic (MHD) turbulence allows the diagnosi...

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Detalles Bibliográficos
Autores principales: Santos-Lima, R., de Gouveia Dal Pino, E.M., Falceta-Gonçalves, D.A., Nakwacki, M.S., Kowal, G.
Formato: JOUR
Materias:
Galaxies: clusters: intracluster medium
Magnetic fields
Methods: numerical
Turbulence
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00358711_v465_n4_p4866_SantosLima
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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