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Monthly Notices of the Royal Astronomical Society(3)
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Cuerpos y fenómenos celestes específicos(3)
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scopus(4)
Absorption spectra from galactic wind models: a framework to link PLUTO simulations to TRIDENT
Conference ObjectAbstract: Galactic winds probe how feedback regulates the mass and metallicity of galaxies. Galactic winds havPalabras claves:Galaxy: halo, hydrodynamics, ISM: evolution, methods: numericalAutores:Brighenti F., Brüggen M., Casavecchia B., 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 - I. Cloud layers with lognormal density distributions
ArticleAbstract: We report three-dimensional hydrodynamical simulations of shocks (Mshock ≥ 4) interacting with fractPalabras claves:galaxies: ISM, galaxies: starburst, hydrodynamics, ISM: clouds, methods: numerical, TurbulenceAutores:Brüggen M., Cottle J., Federrath C., Scannapieco E., Wagner A.Y., Wladimir E. Banda-BarragánFuentes:scopusStructure and kinematics of shocked gas in Sgr B2: Further evidence of a cloud-cloud collision from SiO emission maps
ArticleAbstract: We present SiO J = 2-1 maps of the Sgr B2 molecular cloud, which show shocked gas with a turbulent sPalabras claves:Galaxy: centre, ISM: clouds, ISM: molecules, methods: numericalAutores:Dénes H., Federrath C., J. Armijos-Abendaño, Martín-Pintado J., Requena-Torres M.A., Wladimir E. Banda-BarragánFuentes:scopus