Showing 1–19 of 19 results
/ Date/ Name
Sep 21, 2020Leveraging HST with MUSE: II. Na-abundance variations in intermediate age star clustersSep 7, 2020Leveraging HST with MUSE: I. Sodium abundance variations within the 2 Gyr-old cluster NGC 1978Feb 6, 2019Spectroscopic detection of multiple populations in the ~2 Gyr old cluster Hodge 6 in the LMCSep 6, 2023A closer look at the binary content of NGC 1850Feb 7, 2023The SPIRou Legacy Survey Rotation period of quiet M dwarfs from circular polarization in near-infrared spectral lines: I. The SPIRou APERO analysisJul 27, 2018Extended Main Sequence Turnoffs in Open Clusters as Seen by Gaia: I. NGC 2818 and the Role of Stellar RotationApr 11, 2018The search for multiple populations in Magellanic Cloud Clusters IV: Coeval multiple stellar populations in the young star cluster NGC 1978Jun 7, 2019The search for multiple populations in Magellanic Clouds clusters - V. Correlation between cluster age and abundance spreadsMar 14, 2017The Search for Multiple Populations in Magellanic Cloud Clusters III: No evidence for Multiple Populations in the SMC cluster NGC 419Nov 12, 2021A black hole detected in the young massive LMC cluster NGC 1850Sep 20, 2022CLusters in the Uv as EngineS (CLUES): I. Survey presentation \& FUV spectral analysis of the stellar lightMar 14, 2023Search strategies for supermassive stars in young clusters and application to nearby galaxiesAug 20, 2020SPIRou: nIR velocimetry & spectropolarimetry at the CFHTNov 5, 2019Extended main sequence turnoffs in open clusters as seen by Gaia -- II. The enigma of NGC 2509Jan 6, 2020The WAGGS project -- III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicityApr 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 stars