Modeling the spatial structure of debris disks

Details Modeling the spatial structure of debris disks Modeling the spatial structure of debris disks

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..678e&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.678

Computer Science

Scientific paper

We present high spatial resolution observations and detailed multi-wavelength modeling of the structure and composition of two prominent debris disks and a systematic study on the observability of planet-disk interaction in debris disks with present and future instruments. As the spatial structure of debris disks is, in addition to stellar gravity and radiation, mainly influenced by planet-disk interaction, modeling this structure puts strong constraints on the planetary systems the disks are associated with.

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