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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:scopusShock-multicloud interactions in galactic outflows - II. Radiative fractal clouds and cold gas thermodynamics
ArticleAbstract: Galactic winds are crucial to the cosmic cycle of matter, transporting material out of the dense regPalabras claves:galaxies: ISM, galaxies: starburst, hydrodynamics, ISM: clouds, methods: numerical, TurbulenceAutores:Brüggen M., Cottle J., Federrath C., Heesen V., Scannapieco E., Wagner A.Y., Wladimir E. Banda-BarragánFuentes:scopus