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The protostar FU Orionis may not be bursting: dramatic accretion suppression in embedded young eccentric binaries
In 1936, the protostar FU Orionis began to brighten. Two years later, it was 100 times brighter and has not dimmed since. This object defined the class of FUor-type accretion bursts in protostars. Previous attempts to model FUors simulate isolated protostellar discs, thereby limiting the mass availa
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