Showing 21–40 of 42 results
/ Date/ Name
Jan 19, 2021The properties of clusters, and the orientation of magnetic fields relative to filaments, in magnetohydrodynamic simulations of colliding cloudsApr 4, 2013The Plateau de Bure + 30m Arcsecond Whirlpool Survey reveals a thick disk of diffuse molecular gas in the M51 galaxyJan 9, 2012The Myth of the Molecular RingJan 9, 2017The PdBI Arcsecond Whirlpool Survey (PAWS). The Role of Spiral Arms in Cloud and Star FormationSep 18, 2017The Young Star Cluster population of M51 with LEGUS: I. A comprehensive study of cluster formation and evolutionSep 1, 2016The properties, origin and evolution of stellar clusters in galaxy simulations and observationsSep 27, 2005Spiral shocks, triggering of star formation and the velocity dispersion in Giant Molecular CloudsFeb 5, 2006Spurs and feathering in spiral galaxiesDec 7, 2009Simulations of the grand design galaxy M51: a case study for analysing tidally induced spiral structureMar 8, 2016What can simulated molecular clouds tell us about real molecular clouds?May 4, 2022The SEDIGISM survey: Molecular cloud morphology. II. Integrated source propertiesDec 14, 2018The Spatial Relation between Young Star Clusters and Molecular Clouds in M 51 with LEGUSJan 31, 2019Star Cluster Catalogs for the LEGUS Dwarf GalaxiesMar 20, 2013The Exciting Lives of Giant Molecular CloudsSep 16, 2020The role of collision speed, cloud density, and turbulence in the formation of young massive clusters via cloud-cloud collisionsMar 11, 2019Comparing the Properties of GMCs in M33 from Simulations and ObservationsDec 2, 2020The SEDIGISM survey: Molecular clouds in the inner GalaxyAug 31, 2022The formation of clusters and OB associations in different density spiral arm environmentsSep 24, 2013The dependence of stellar age distributions on GMC environmentMar 24, 2009A Simple Model for the Relationship Between Star Formation and Surface Density