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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: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:scopus