机译:Sustaining star formation rates in spiral galaxies: Supernova-driven turbulent accretion disk models applied to THINGS galaxies
CDS, Observatoire Astronomique, UMR 7550, 11 Rue de l'université, 67000 Strasbourg, France;
National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, United States;