Figure 9.
Evolution of individual sink particle masses for three inclinations of runs B3M…I…. The higher the inclination, the later star formation begins. In addition, the star formation rate and efficiency are strongly influenced (see also Fig. 1).
Evolution of individual sink particle masses for three inclinations of runs B3M…I…. The higher the inclination, the later star formation begins. In addition, the star formation rate and efficiency are strongly influenced (see also Fig. 1).
