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- W2045012679 abstract "We investigate the relativistic acceleration and collimation of a wind launched from a magnetized accretion disk corona. Time-dependent simulations of the full set of special relativistic magnetohydrodynamic (RMHD) equations are performed with the publicly available PLUTO 1 code. In order to provide an injection boundary in dynamical equilibrium, Newtoninan gravity was added as a source term. The flow starts out with sub-escape velocity and we allow for sub-magnetoslow injection to consistently prescribe the mass-loading. The detailed trans-field and parallel-field force-balances are shown with highlights on the relativistic contribution due to electric fields. 2 Generally we find collimated flows with mass-weighted half-opening angles of 3–7 degrees and mildly relativistic velocities. The outer subrelativistic flow is a promising candidate for the X–ray absorption winds that are observed in many radio-quiet active galactic nulei (AGN)." @default.
- W2045012679 created "2016-06-24" @default.
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- W2045012679 date "2010-06-01" @default.
- W2045012679 modified "2023-09-26" @default.
- W2045012679 title "FROM DISK WINDS TO RELATIVISTIC JETS" @default.
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- W2045012679 doi "https://doi.org/10.1142/s0218271810016907" @default.
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