Hydrodynamical simulations show that high prograde initial stellar spin recovers the dimming trend in rpTDE outbursts, supporting the Hills mechanism for orbit placement.
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Radiation hydrodynamic simulations of wind-reprocessed TDEs reveal a ~3-week offset between optical/UV and bolometric light curve peaks due to the buildup time of the reprocessing layer.
citing papers explorer
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The Role of Stellar Spin in Repeating Partial Tidal Disruption Events
Hydrodynamical simulations show that high prograde initial stellar spin recovers the dimming trend in rpTDE outbursts, supporting the Hills mechanism for orbit placement.
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The Light Curve of Wind-Reprocessed Tidal Disruption Events
Radiation hydrodynamic simulations of wind-reprocessed TDEs reveal a ~3-week offset between optical/UV and bolometric light curve peaks due to the buildup time of the reprocessing layer.