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Hubert KLAHR

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2D axissymetric Pluto Simulation: Temperature<br />

due to irradiation from star and thermal<br />

relaxation tau = 0.1 (also works for flux limited<br />

diffusion in irradiated disks)<br />

• eeeeeeee<br />

Star-><br />

Thermal wind:<br />

See Nelson, Gressel &<br />

12/13/2009 <strong>Hubert</strong> Klahr - Planet Formation Umurhan - MPIA astro-ph 46<br />

Heidelberg

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