Figure 5:
Instability regions of the system in Table 1 for different contact ratios. ε=ε1=ε2=0.3 (g=1). The planets are equally spaced with in–phase meshes (γsn=γrn=0). (a) γsr=0, (b) γsr=1/2.
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OSU0907_Fig5
Figure 5:
Instability regions of the system in Table 1 for different contact ratios. ε=ε1=ε2=0.3 (g=1). The planets are equally spaced with in–phase meshes (γsn=γrn=0). (a) γsr=0, (b) γsr=1/2.
Figure 5:
Instability regions of the system in Table 1 for different contact ratios. ε=ε1=ε2=0.3 (g=1). The planets are equally spaced with in–phase meshes (γsn=γrn=0). (a) γsr=0, (b) γsr=1/2.
