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Agnieszka Janiuk,Konstantinos Sapountzis,Jeremy Mortier,Ireneusz Janiuk
Pág. 86 - 102
We model the structure and evolution of black hole accretion disks using numerical simulations. The numerics is governed by the equations of general relativistic magneto-hydrodynamics (GRMHD). Accretion disks and outflows can be found at the base of very...
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