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We explore the Gaia DR2 proper motions of six young, main-sequence stars,members of the Large Magellanic Cloud (LMC) reported by Moni Bidin et al.(2017). These stars are located in the outskirts of the disk, between 7 and 13degrees from the LMC's center where there is very low H I content. Gaia DR2proper motions confirm that four stars formed locally, in situ, while two areconsistent with being expelled via dynamical interactions from inner, moregas-rich regions of the LMC. This finding establishes that recent starformation occurred in the periphery of the LMC, where thus far only oldpopulations are known.

In-Situ Star Formation in the Outskirts of the Large Magellanic Cloud: Gaia DR2 Confirmation