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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Numerical simulations identify a sharp transition between runaway disruption and stable eccentric mass transfer in star-black hole binaries set by pericenter distance.
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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Bridging Roche Lobe Overflow and micro-TDEs: The Runaway Evolution of Eccentric Mass Transfer in Star-Black Hole Binaries
Numerical simulations identify a sharp transition between runaway disruption and stable eccentric mass transfer in star-black hole binaries set by pericenter distance.