Using Disk Morphology to Constrain the Orbit of HD 106906b
Abstract: Debris disks are collections of dust around main sequence stars, formed through collisions of planetesimals such as comets and asteroids. Although debris disks are common, only a handful of systems include a disk as well as a directly imaged planet. HD 106906 is a short-period stellar binary, host to an 11 Mjup planet, HD … Read more