作者: S. Massaglia , P. Rossi , G. Bodo , C. Zanni , A. Ferrari
DOI:
关键词:
摘要: We present numerical time-dependent MHD simulations of the acceleration and collimation process astrophysical jets from accretion disks. begin to perform a parameter space analysis by varying amount resistivity introduced in disk allow steady motion. The aim this work is study effect determining properties both ejection flows.