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Monthly Notices of the Royal Astronomical Society(3)
Proceedings of the International Astronomical Union(2)
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: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:scopus