About 5 LMC globular clusters move significantly differently from surrounding red-clump disk stars, and these outliers can bias LMC enclosed-mass estimates by up to 30%.
R., Origlia, L., & Pecci, F
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A Statistical Framework to Identify Kinematically Outlying LMC Globular Clusters and Implications for the LMC's Dark Matter Profile
About 5 LMC globular clusters move significantly differently from surrounding red-clump disk stars, and these outliers can bias LMC enclosed-mass estimates by up to 30%.