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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Dust-free inner disk regions around Herbig stars are molecular-rich environments that dominate CO and H2O line emission between 1 and 28 microns and produce detectable SiO overtone lines.
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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Gas chemistry in the dust depleted inner regions of protoplanetary disks. I. Near-IR spectra and overtones
Dust-free inner disk regions around Herbig stars are molecular-rich environments that dominate CO and H2O line emission between 1 and 28 microns and produce detectable SiO overtone lines.