The growth of spheroidal components in numerical simulations

The origin of the disk and spheroid of galaxies is a key open question in understanding their morphologies and evolutions. Using numerical simulations, we can explore kinematically decomposed disk and spheroidal components in detail. I will show some recent works and my preliminary work on this topic.

Discussion Leader: 
Min Du
Place: 
KIAA-PKU
Time: 
Tuesday, May 14, 2019 - 12:00pm