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Filament formation in wind-cloud interactions - I. Spherical clouds in uniform magnetic fields
ArticleAbstract: Filamentary structures are ubiquitous in the interstellar medium, yet their formation, internal struPalabras claves:galaxies: starburst, ISM: clouds, ISM: Magnetic fields, MHD- methods: numerical, Stars: winds, outflowsAutores:Bicknel G.V., Crocker R.M., Federrath C., Parkin E.R., Wladimir E. Banda-BarragánFuentes:scopusFilament formation in wind-cloud interactions- II. Clouds with turbulent density, velocity, and magnetic fields
ArticleAbstract: We present a set of numerical experiments designed to systematically investigate how turbulence andPalabras claves:galaxies: starburst, ISM: clouds, ISM: Magnetic fields, methods: numerical, MHD, TurbulenceAutores:Bicknell G.V., Crocker R.M., Federrath C., Wladimir E. Banda-BarragánFuentes:scopusModeling a propulsion system for the trajectory correction of weather balloons
Conference ObjectAbstract: We present a mathematical framework that helps in the design of an electric propulsion system that uPalabras claves:Autores:Daniel Vera Hensiek, Ericson D. Lopez, Esteban Valencia, Wladimir E. Banda-BarragánFuentes:googlescopusMorphology 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: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: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: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:scopusThe Launching of Cold Clouds by Galaxy Outflows. III. The Influence of Magnetic Fields
ArticleAbstract: Motivated by observations of outflowing galaxies, we investigate the combined impact of magnetic fiePalabras claves:Autores:Brüggen M., Cottle J., Federrath C., Scannapieco E., Wladimir E. Banda-BarragánFuentes:scopus