A firm prediction from theory is that the inflow of gas onto galaxies, which acts as a fuel for star formation, and the outflow of chemically-enriched material from star forming regions are key drivers of galaxy evolution. Therefore the study of the intergalactic medium (IGM) and of the regions
Novel astrophysical probes of dark matter
Space weather and the solid Earth: the hazard to technology at the Earth’s surface
Is the study of the CGM fulfilling its promise of revealing the processes that drive galaxy evolution?