期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 380, 期 2, 页码 646-656出版社
BLACKWELL PUBLISHING
DOI: 10.1111/j.1365-2966.2007.12099.x
关键词
stars : formation; supernovae : general; galaxies : formation; galaxies : ISM
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.
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