Oral title: Circumplanetary Disk Simulations Preparing the Observations

Oral abstract: It is now possible to detect the circumplanetary disks formed around giant 
planets. These disks are particular interest as they regulate the late accretion to the 
planet and are the birthplaces for satellites. 
With a suite of radiative hydrodynamic simulations, we explore the characteristics of 
circumplanetary disk around planets with various masses to provide model predictions for 
observations.