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Young, Massive Star Clusters in the Antennae
2008While massive star clusters have been detected in almost every galaxy with appreciable star formation, they are most prevalent in interacting and merging galaxies. As many as 95% of these clusters will ultimately be disrupted, often in the first 10 Myr, but those clusters that do survive may be the progenitors of globular clusters.
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Massive binary stars and the kinematics of Young Massive Clusters
2013Located in the Large Magellanic Cloud, R136 is a rare example of a nearby young and dense massive star cluster in which individual stars can be resolved. Often suggested as a globular cluster in formation, its study is of great interest and promises to provide insights into the early dynamical evolution of massive star clusters.
Henault-Brunet, Vincent, Brunet, Vincent
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Intermediate mass black hole formation in compact young massive star clusters
Monthly Notices of the Royal Astronomical Society, 2021Thorsten Naab +2 more
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Formation and evolution of young massive clusters in galaxy mergers: the SMUGGLE view
Monthly Notices of the Royal Astronomical Society, 2022Hui Li +2 more
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The early evolution of young massive clusters
Astronomy and Astrophysics, 2023M Stoop, A de Koter, H J G L M Lamers
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Gas expulsion and the destruction of massive young clusters
Monthly Notices of the Royal Astronomical Society, 2006Simon P Goodwin, Nate Bastian
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