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Infuence of volatiles transport in disks on giant planets composition

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Figure 1.1: The disk's response to a Green's function source, from Armitage (2010). Mass is accreted inward, but angular momentum in transported outward.
Table 2.1: The observed properties of protoplanetary disks DM Tau and GM Aur, from Hueso &
Figure 1.2: The observed disks frequency as a function of their age, from Hernández et al
Figure 1.4: The temperature proles corresponding to the models tting the DM tau observations, from Hueso & Guillot (2005).
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