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Morphology of radio relics-I. What causes the substructure of synchrotron emission?
ArticleAbstract: High-resolution radio observations of cluster radio relics often show complex spatial and spectral fPalabras claves:acceleration of particles, galaxies: clusters: intracluster medium, methods: numerical, Shock wavesAutores:Brüggen M., Domínguez-Fernández P., Mignone A., Mukherjee D., Rajpurohit K., Vaidya B., Vazza F., Wladimir E. Banda-BarragánFuentes:scopusMorphology of radio relics-II. Properties of polarized emission
ArticleAbstract: Radio relics are diffuse radio sources in galaxy clusters that are associated with merger shock wavePalabras claves:acceleration of particles, galaxies: clusters: intracluster medium, Intergalactic medium, methods: numerical, MHD, Shock wavesAutores:Brüggen M., Domínguez-Fernández P., Hoeft M., Mignone A., Mukherjee D., Rajpurohit K., Vaidya B., Vazza F., Wittor D., Wladimir E. Banda-BarragánFuentes:scopusOn the dynamics and survival of fractal clouds in galactic winds
ArticleAbstract: Recent observations suggest that dense gas clouds can survive even in hot galactic winds. Here we shPalabras claves:galaxies: ISM, galaxies: starburst, hydrodynamics, ISM: clouds, methods: numerical, TurbulenceAutores:Brüggen M., F. J. Zertuche, Federrath C., Javier García-del-Valle, Wagner A.Y., Wladimir E. Banda-BarragánFuentes:scopus