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Figure 2: Same as Fig. 1 for planet's eccentricity equal to 0.1 |
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Figure 3: Same as Fig. 1 for the 5:7 resonance |
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Figure 4:
Same as Fig. 1 for the 7:9 resonance and different planetary masses.
Dashes stand for planet's mass equal to
|
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Figure 6: Same as Fig. 1, with continuous line standing for the generic method |
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Figure 7: Same as Fig. 6, for the 5:7 extended resonance |
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Figure 8:
Corotation points for the 7:9 resonance, for the generic method, planet
as in Fig. 1, except for planetary masses. Continuous line stands for planet's mass equal to
|
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Figure 9:
Corotation points for the 4:7 resonance, for the generic method, planet
as in Fig. 1, except for planetary masses.
Dots stand for planet's mass equal to
|
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Figure 10: Corotation points for the 3:2 resonance, for the generic method, planet as in Fig. 5. Continuous line and circles stand for points determined considering Stokes drag (generic and numerical methods) while dashes stand for v2 drag |
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Figure 14: Variation of corotation points for the case of Stokes drag, with planet's mass for the 3:2 resonance, generic method with planet, except for masses, as in Fig. 5 |
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Figure 15: Variation of corotation points for the case of Stokes drag, with planet's eccentricity, for the 3:2 resonance, generic method with planet, except for eccentricities, as in Fig. 5 |
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Figure 16:
Corotation points for the 11:10 interior resonance, Stokes drag,
generic method, with
|
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Figure 17: Same as Fig. 16 for the 9:8 resonance, only generic method |
Copyright ESO 2001