YSO jet diversity, including counter-rotating and choked jets, arises from a spine-tower balance controlled by stellar rotation and magnetospheric field strength.
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GRRMHD simulations of CEM-adapted tori find thermal instability in 17-46 days with spin-dependent X-ray decline and soft excess matching AT2021ehb observations.
citing papers explorer
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Modeling YSO Jets in 3D III: Dependence of Accretion and Jet Properties on Stellar Magnetospheric Field Strength and Rotation
YSO jet diversity, including counter-rotating and choked jets, arises from a spine-tower balance controlled by stellar rotation and magnetospheric field strength.
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GRRMHD Simulations of State Transitions in Non-Jetted Tidal Disruption Events
GRRMHD simulations of CEM-adapted tori find thermal instability in 17-46 days with spin-dependent X-ray decline and soft excess matching AT2021ehb observations.