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From Protoplanetary to Debris Disks
2002We 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.
Dominik, C., Dullemond, C.P.
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Dynamical Processes in Debris Disks
EAS Publications Series, 2010Debris disks are dusty and/or gasous disk that are viewed in scattered light and thermal emission around stars around 10 7 –10 8 yr. It is well known that the dust in these system is not primodial. It is short lived and must be continuously replenished by colliding planetesimals.
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Debris Disks: Structure, Composition, and Variability
Annual Review of Astronomy and Astrophysics, 2018A Meredith Hughes +2 more
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Hot grain dynamics by electric charging and magnetic trapping in debris disks
Planetary and Space Science, 2020Takeru Suzuki +2 more
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Searching for debris disks around isolated pulsars
Planetary and Space Science, 2014Zhongxiang Wang
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