Showing 1–20 of 42 results
/ Date/ Name
Jan 12, 2011Was a cloud-cloud collision the trigger of the recent star formation in Serpens?Feb 5, 2010Pattern speeds in interacting galaxiesMay 11, 2018Simulations of the flocculent spiral M33: what drives the spiral structure?Apr 20, 2020The formation of young massive clusters by colliding flowsOct 18, 2021The formation of massive stellar clusters in converging galactic flows with photoionisationDec 9, 2021Grouped star formation: converting sink particles to stars in hydrodynamical simulationsFeb 5, 2006The formation of molecular clouds in spiral galaxiesJul 8, 2010Age distributions of star clusters in spiral and barred galaxies as a test for theories of spiral structureMar 4, 2022The SEDIGISM survey: Molecular cloud morphology. I. Classification and star formationJun 21, 2012Giant Molecular clouds: what are they made from, and how do they get there?Sep 23, 2019The evolution of pitch angles of spiral armsJul 19, 2016Magnetic field evolution and reversals in spiral galaxiesDec 8, 2014Synthetic CO, H2 and HI surveys of the Galactic 2nd Quadrant, and the properties of molecular gasNov 4, 2014The frequency and nature of `cloud-cloud collisions' in galaxiesJun 16, 2017The evolution of Giant Molecular FilamentsJan 17, 2017SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar mediumJul 1, 2011The properties of the ISM in disc galaxies with stellar feedbackJan 7, 2019Simulating the impact of the Smith CloudAug 25, 2009Hydrodynamic Simulations of M51 and the interaction with NGC 5195Jan 18, 2011Why are most molecular clouds not gravitationally bound?