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Disc galaxy evolution along the Hubble sequence
Authors:Marios Kampakoglou  Joseph Silk
Institution:Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH
Abstract:Galaxy discs are characterized by star formation histories that vary systematically along the Hubble sequence. We study global star formation, incorporating supernova feedback, gas accretion and enriched outflows in discs modelled by a multiphase interstellar medium in a fixed gravitational potential. The star formation histories, gas distributions and chemical evolution can be explained in a simple sequence of models which are primarily regulated by the cold gas accretion history.
Keywords:stars: formation  supernovae: general  galaxies: formation  galaxies: ISM
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