Expositor: Massimiliano Parente (SISSA – INAF, Trieste, Italia)

Fecha: viernes 1 de diciembre, 11 hs

Resumen: Dust grains play a pivotal role, although still poorly understood, in the broader context of galaxy evolution. I will discuss the study of dust within this field by means of hydrodynamical simulations and semi-analytic models of galaxy evolution. I will present some key results of our group over recent years, encompassing predictions about grains properties, the overall dust abundance of the Universe and the dust content of different cosmic web environments. Finally, I will provide a brief overview of future and ongoing projects.

Esperamos vuestra participación este viernes en el auditorio del IATE.
Se podrá participar virtualmente mediante el enlace: https://meet.google.com/hgu-akrs-xvc