Authors compute FUV fluxes for ~8600 Orion stars via 3D sub-cluster geometry and find Ha accretion signatures decline faster in high-FUV regions, broadly matching external photoevaporation models but without firm confirmation.
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Far-ultraviolet flux distribution in Orion and its relation to stellar accretion
Authors compute FUV fluxes for ~8600 Orion stars via 3D sub-cluster geometry and find Ha accretion signatures decline faster in high-FUV regions, broadly matching external photoevaporation models but without firm confirmation.