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SUMMARY:Review - models of protoplanetary disks - Dominik\, C (Amsterdam)
DTSTART:20090817T130000Z
DTEND:20090817T134000Z
UID:TALK19509@talks.cam.ac.uk
CONTACT:Mustapha Amrani
DESCRIPTION:In my talk I will address a variety of modeling approaches to 
 protoplanetary disks. I will discuss radiative transfer models that are us
 ed to derive spectral energy distributions and address the issues related 
 to various geometrical structures in such disks and the pitfall of modelin
 g these with codes not appropriate for complex geometries. I will discuss 
 the latest models of the inner boundary of protoplanetary disks near the d
 ust evaporation zone and show that a detailed treatment of the evaporation
  physics leads to interesting structure\, size and chemical sorting\, and 
 possibly to instabilities as a source for observational variability\, both
  in SED features and in interferometric observations. I will also discuss 
 the latest suite of models covering dust settling and coagulation on a glo
 bal scale in disks. Hydrodynamic and magnetohyrdodynamic models are beyond
  the scope of this review talk.
LOCATION:Seminar Room 1 Newton Institute
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