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From Protoplanetary to Debris Disks

  • Carsten Dominik
  • Cornelius P. Dullemond
Conference paper
Part of the ESO Astrophysics Symposia book series (ESO)

Abstract

We discuss the physical difference between protoplanetary and debris (Vega-like) disks and consider the course of evolution which leads from the first to the latter. We discuss a simple evolutionary model for debris disks and predict 20μm fluxes for future observations with VISIR.

Keywords

Radiation Pressure Settling Time Circumstellar Disk Dust Masse Debris Disk 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2002

Authors and Affiliations

  • Carsten Dominik
    • 1
  • Cornelius P. Dullemond
    • 2
  1. 1.Sterrenkundig Instituut “Anton Pannekoek”AmsterdamNetherlands
  2. 2.Max-Planck-Institut für AstrophysikGarchingGermany

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