Bekki, KenjiCouch, WarrickBeasley, MichaelForbes, Duncan AChiba, MasashiDa Costa, Gary2015-12-130004-637Xhttp://hdl.handle.net/1885/86795The Large Magellanic Cloud (LMC) has a unique cluster formation history in that nearly all of its globular clusters were formed either ∼13 Gyr ago or less than ∼3 Gyr ago. It is not clear what physical mechanism is responsible for the most recent clusKeywords: Galaxies: interactions; Galaxies: star clusters; Galaxies: stellar content; Magellanic Clouds200410.1086/4233722015-12-12