Showing 21–37 of 37 results
/ Date/ Name
Apr 15, 2014Constraining globular cluster formation through studies of young massive clusters - II. A Single Stellar Population Young Massive Cluster in NGC 34Jul 27, 2018Extended Main Sequence Turnoffs in Open Clusters as Seen by Gaia: I. NGC 2818 and the Role of Stellar RotationNov 3, 2017Interpreting the complex CMDs of the Magellanic Clouds clustersMay 5, 2016Searching for GC-like abundance patterns in young massive clustersDec 1, 2016The Search for Multiple Populations in Magellanic Cloud Clusters II: The Detection of Multiple Populations in Three Intermediate-Age SMC ClustersSep 19, 2013Constraining Globular Cluster Formation Through Studies of Young Massive Clusters: I. A lack of ongoing star formation within young clustersApr 11, 2018The search for multiple populations in Magellanic Cloud Clusters IV: Coeval multiple stellar populations in the young star cluster NGC 1978Apr 17, 2024The 33 M$_\odot$ black hole Gaia BH3 is part of the disrupted ED-2 star clusterJan 22, 2015Constraining globular cluster formation through studies of young massive clusters - V. ALMA observations of clusters in the AntennaeNov 5, 2019Extended main sequence turnoffs in open clusters as seen by Gaia -- II. The enigma of NGC 2509Oct 24, 2022High-precision abundances of first population stars in NGC 2808: confirmation of a metallicity spreadMar 3, 2020Chromosome maps of young LMC clusters: An additional case of coeval multiple populationsApr 20, 2020Searching for globular cluster chemical anomalies on the main sequence of a young massive clusterSep 14, 2021Exploring the role of binarity in the origin of the bimodal rotational velocity distribution in stellar clustersOct 2, 2017Age as a Major Factor in the Onset of Multiple Populations in Stellar ClustersNov 21, 2016A high fraction of Be stars in young massive clusters: evidence for a large population of near-critically rotating starsOct 28, 2015Controversial Age Spreads from the Main Sequence Turn-Off and Red Clump in Intermediate-Age Clusters in the LMC