TY - CONF T1 - Large resistivity in numerical simulations of radially self-similar outflows Y1 - 2011 A1 - Čemeljić, Miljenko A1 - Vlahakis, Nektarios A1 - Tsinganos, Kanaris KW - magnetic fields (magnetohydrodynamics): MHD KW - methods: numerical KW - outflows KW - stars: winds AB - We investigate conditions in a radially self-similar outflow in the regime of large resistivity. Using the PLUTO code, we performed simulations with proper choice of boundary conditions, relaxed at the footpoints of critical surfaces in the flow. We investigate outflow propagation in a high-resistive disk corona, and compare it to the results with small or vanishing resistivity. VL - 271 SN - 1743-9221 UR - https://ui.adsabs.harvard.edu/abs/2011IAUS..271..371C JO - Astrophysical Dynamics: From Stars to Galaxies ER -