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The impact of turbulence and magnetic field orientation on star forming filaments, and . (Mar 5, 2015)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.StarBench: The D-type expansion of an HII region, , , , , , , , , and 9 other author(s). (2015)cite arxiv:1507.05621Comment: 20 pages, 12 Figures, 4 Tables. Accepted for publication in MNRAS. Comments are welcome. Participation in future StarBench tests is also welcome.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.Is molecular cloud turbulence driven by external supernova explosions?, , , , and . (Feb 3, 2018)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.The energy and momentum input of supernova explosions in structured and ionised molecular clouds, and . (2014)cite arxiv:1410.0011Comment: 15 pages, 9 figures; submitted to MNRAS; comments welcome.Model calculations of the electron affinities and ionization potentials of DNA. Chem.\,Phys.\,Lett., (2003)On correlation in the first row transition metal atoms, , and . J. Chem. Phys., (1982)