Mapping the Hot Phase of CGMs in Nearby Galaxies

Mapping the Hot Phase of CGMs in Nearby Galaxies

Mapping the circumgalactic medium (CGM) in emission is one of the important scientific goals for astronomers to either use the modern ground-based telescopes or the future space missions.  CGMs are multi-phases, key to understand  the galaxy ecosystem and its accretion and feedback. In this talk, I will introduce a few scientific projects in our group for the efforts in understanding the mechanims of the hot diffuse emission in nearby universe with high spectral resolution data X-ray. In addition, I will introduce the prospective X-ray mission in the near future in China.

Sebastián López
Colloquium  Coordinator
DAS/UChile  – slopez@das.uchile.cl