Determining the Origin of Inner Planetary System Debris Orbiting the Dustiest Main Sequence Stars
Abstract
We develop a means to distinguish between warm dusty circumstellar debris disks produced by steady state collisional evolution of a planetesimal belt or through transient events.
- Publication:
-
Formation, Detection, and Characterization of Extrasolar Habitable Planets
- Pub Date:
- April 2014
- DOI:
- Bibcode:
- 2014IAUS..293..273M
- Keywords:
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- planets and satellites: formation;
- circumstellar matter;
- planetary systems: formation