IN BRIEF<.1.) STUDY THE EVOLUTION OF CIRCUMBINARY NEBULAE USING 3D RADIATIVE DISK MODELS .2.) STUDY PLANET MIGRATION IN THESE DISKS FOR DIFFERENT ORBITAL INCLINATIONS AND MASSES OF THE PLANET AND.3.) STUDY THE CAPTURE OF CBPS BETWEEN MMRS AND IN PROXIMITY OF THE BINARY'S BOUNDARY OF STABILITY IN TERMS OF THE PHYSICAL CHARACTERISTICS OF THE DISK IN PARTICULAR THE SIZE OF ITS INNER CAVITY AND MAKE STATISTICAL PREDICTIONS ABOUT PLANET TRAPPING.
$106,988FY2021National Aeronautics and Space AdministrationNASA
Planetary Science Institute, Tucson AZ