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A cloud-cloud collision in Sgr B2? 3D simulations meet SiO observations
Conference ObjectAbstract: We compare the properties of shocked gas in Sgr B2 with maps obtained from 3D simulations of a colliPalabras claves:Galaxy: centre, hydrodynamics, ISM: clouds, radio lines: ISMAutores:Dénes H., Helga Dénes, J. Armijos-Abendaño, Jairo Armijos, Wladimir E. Banda-BarragánFuentes:googlescopusAbsorption 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:scopusFilament 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:scopusMorphology 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: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:googlescopusShock-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:scopus