A low-mass object embedded in a magnetized disk forms an MRI-turbulent mini-accretion disk that amplifies its magnetic field and launches collimated bipolar jets that exceed the local escape speed.
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Global simulations of accretion flows onto perturbers embedded in magnetized disks -I. MRI and jet formation in ideal MHD
A low-mass object embedded in a magnetized disk forms an MRI-turbulent mini-accretion disk that amplifies its magnetic field and launches collimated bipolar jets that exceed the local escape speed.