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Supernova-driven outflows in NGC 7552: a comparison of H α and UV tracersThe dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an endThe impact of angular momentum on black hole accretion rates in simulations of galaxy formationGalaxy size trends as a consequence of cosmologyWhich galaxies dominate the neutral gas content of the Universe?The origin of the atomic and molecular gas contents of early-type galaxies – II. Misaligned gas accretionOn the connection between the metal-enriched intergalactic medium and galaxies: an O vi–galaxy cross-correlation study atz< 1A compact, metal-rich, kpc-scale outflow in FBQS J0209−0438: detailed diagnostics from HST/COS extreme UV observationsThe evolution of the star-forming sequence in hierarchical galaxy formation modelsA dynamical model of supernova feedback: gas outflows from the interstellar mediumThe metallicity of galactic windsChemodynamical Simulations of Dwarf Galaxy Evolution
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description
im Januar 2013 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в січні 2013
@uk
name
How supernova explosions power galactic winds
@en
How supernova explosions power galactic winds
@nl
type
label
How supernova explosions power galactic winds
@en
How supernova explosions power galactic winds
@nl
prefLabel
How supernova explosions power galactic winds
@en
How supernova explosions power galactic winds
@nl
P2860
P356
P1476
How supernova explosions power galactic winds
@en
P2093
Richard G. Bower
P2860
P304
P356
10.1093/MNRAS/STS439
P407
P577
2013-01-03T00:00:00Z
P818
P819
2013MNRAS.429.1922C