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The SILCC project: III. Regulation of star formation and outflows by stellar winds and supernovae, , , , , , , , , and 2 other author(s). (2016)cite arxiv:1606.05346Comment: 23 pages; submitted to MNRAS.A comparison of the Milky Way's recent star formation revealed by dust thermal emission and high-mass stars, , , , , , , , , and 3 other author(s). (2023)cite arxiv:2308.01330Comment: Submitted to A&A (31JUL2023). 8 pages, 7 figures. Comments are welcome.Is molecular gas necessary for star formation?, and . (2011)cite arxiv:1105.3073 Comment: 11 pages, 7 figures. Submitted to MNRAS.The Chemistry of the Early Universe. (2011)cite arxiv:1107.3314Comment: 12 pages, to appear in the proceedings of IAU Symposium 280: "The Molecular Universe".New ALMA constraints on the star-forming ISM at low metallicity: A 50 pc view of the blue compact dwarf galaxy SBS0335-052, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1702.08467Comment: accepted for publication in MNRAS.Modelling the supernova-driven ISM in different environments, , , , , , , , , and 4 other author(s). (2014)cite arxiv:1411.0009Comment: 18 pages, 12 figures, 2 tables. Submitted to MNRAS.The SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM, , , , , , , , , and . (2014)cite arxiv:1412.2749Comment: 30 pages, 23 figures, submitted to MNRAS. Comments welcome! For movies of the simulations and download of selected Flash data see the SILCC website: http://www.astro.uni-koeln.de/silcc.Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1902.10437Comment: 23 pages, 9 figures, accepted for publication in A&A.