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Theory of planet formation and comparison with observation

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Figure

Figure 1.: Simulation nJ6 of the in-situ formation of Jupiter. Top left: evolution of
Figure 2.: Radius R (dashed), core ra-dius Rcore (solid) and capture radiusRcapt (dotted) as a function of timefor the nJ6 case.The inset figureis a zoom-in onto the late evolutionand shows the radius as found in thiswork (solid line), in BC03 (dashed) andB
Figure 3.:(Total) luminos-
Figure 4.: Temporal evolution of the mass-radius diagram for synthetic planets. TheGreen: 5the panels
+3

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