研究成果藝廊

This figures illustrate density profiles in log scale from simulations of two-temperature model of outflows from a young stellar object. (Left) Mosaic of simulations demonstrating effects of varying temperature and degree of magnetization. Panel indices from (a) to (c) shows decreasing magnetic field strength, and (1) to (3) shows increasing wind temperature. The central axial jet is more collimated and the shell structure is narrowed when the magnetic force is relatively important. (Zeus-TW simulations in Wang et al. 2015)