Description
The physical structure of disks during the early stages of their formation is crucial for understanding the accretion process and planet formation. However, the temperature structure of young disks is still poorly understood. The temperature structure of young disks is an important parameter that is connected to the accretion rate. Furthermore, it also sets the composition of the planet-forming material. In this talk, I will present the models and observational results of the temperature structure of young disks.
