Speaker
Asier Lambarri
Description
Numerical Simulations of the Universe provide a unique laboratory for studying the assembly LSB features around galaxies. Until recently, the resolution of these simulations only allowed to resolve the coarsest LSB structures, but the arrival of Very-High resolution simulations it is becoming possible to resolve stellar stream around massive hosts.
On this talk, we will present preliminary results on the formation of stellar streams on the Vintergatan suite of simulations, where we identify two factors shaping stellar stream formation.
