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Bar Formation by Galaxy-Galaxy Interactions
2004Bar formation process in interacting galaxies is reviewed on the basis of recent numerical simulations. I focus especially on the possible kinematical difference between tidally-induced bars and spontaneous bars: the former spans a wider range in the rotation rate, depending upon the parameters of the interaction as well as the internal structure of ...
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Simulations of the formation, evolution and clustering of galaxies and quasars
Nature, 2005Volker Springel +2 more
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Properties of galaxies reproduced by a hydrodynamic simulation
Nature, 2014Mark Vogelsberger +2 more
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High molecular gas fractions in normal massive star-forming galaxies in the young Universe
Nature, 2010Linda Tacconi +2 more
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Strangulation as the primary mechanism for shutting down star formation in galaxies
Nature, 2015Roberto Maiolino
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Systematic variation of the stellar initial mass function in early-type galaxies
Nature, 2012Michele Cappellari +2 more
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