Physics of Debris Disks

Details Physics of Debris Disks Physics of Debris Disks

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007esasp.643..123k&link_type=abstract

Workshop on Dust in Planetary Systems (ESA SP-643). September 26-30 2005, Kauai, Hawaii. Editors: Krueger, H. and Graps, A., p.1

Physics

1

Scientific paper

In the last decade, hundreds of debris disks around main sequence stars have been detected through infrared excesses in the stellar spectra and some imaged directly. This review outlines essential forces and effects exerted on dust in debris disks and then summarizes key properties of the disks, as determined by these physics. Size and spatial distribution of dust, long- and short-term evolution of disks, as well as interrelations between dust, its parent bodies, and embedded planets are addressed.

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