Physically Consistent Protoplanetary Disk Models

Details Physically Consistent Protoplanetary Disk Models Physically Consistent Protoplanetary Disk Models

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002hst..prop.9524c&link_type=abstract

HST Proposal ID #9524

Physics

Hst Proposal Id #9524 Star Formation

Scientific paper

We propose to make our physically consistent models for protoplanetary disks, which are the most detailed so far, available to the community. We propose to make available two types of models. First, we will construct a complete grid of models where dust and gas are well mixed throughout the disks, which are relevant for the youngest, less evolved objects. Then, we propose to advance in our present modeling efforts to include the effects of dust coagulation and settling towards the midplane on the structure and the emission of the disks. With our results, we propose to create a Web-based library of disk model results, including both scattered light images, as observed by the imaging detectors of HST, and far infrared to millimeter spectral energy distributions, to provide the community with the tools required for a comprehensive interpretation of protoplanetary disk data. Our proposed effort will provide the Star Formation users of HST with a powerful tool to best interpret their data and obtain key results for protoplanetary disk evolution.

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