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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Star formation model choice in galaxy simulations controls giant molecular cloud lifetimes, yielding 20-30 Myr with sink particles versus over 200 Myr with the gravo-thermo-turbulent prescription.
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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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From short-lived to long-lived clouds: impact of star formation models on giant molecular cloud evolution in simulations of an NGC 300-like galaxy
Star formation model choice in galaxy simulations controls giant molecular cloud lifetimes, yielding 20-30 Myr with sink particles versus over 200 Myr with the gravo-thermo-turbulent prescription.