Resolving the inner few AU in protostellar disk simulations yields complete tidal disruption of migrating fragments and shorter, sharper accretion outbursts than coarser 30 AU models.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2representative citing papers
Mid-IR light curves of IRAS20126+4104 confirm a 6.8 yr periodic variation interpreted as evidence that the 12 solar-mass protostar is bloated to a radius of roughly 200 solar radii due to rotation with an obscuring spot.
citing papers explorer
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From Fragments to Flares: Migration, Tidal Disruption, and Observable Bursts in Massive Protostellar Disks
Resolving the inner few AU in protostellar disk simulations yields complete tidal disruption of migrating fragments and shorter, sharper accretion outbursts than coarser 30 AU models.
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Evidence for a bloated massive protostar in IRAS20126+4104
Mid-IR light curves of IRAS20126+4104 confirm a 6.8 yr periodic variation interpreted as evidence that the 12 solar-mass protostar is bloated to a radius of roughly 200 solar radii due to rotation with an obscuring spot.