Is the Fault in their Stars?
Identifying the incidence of AGN as a function of star formation rate
Identifying the incidence of AGN as a function of star formation rate
Is the evolution of galaxies and their AGN driven by past mergers?
A Seyfert 2 galaxy’s energetic nucleus creates impressive twin outflows, but how are they affecting its star formation?
A novel approach to estimate their mass may help reveal the relationship between supermassive black holes and the galaxies they inhabit.
Today’s post presents SIMBA, a cosmological simulation that focuses on understanding the growth and evolution of black holes and their host galaxy.
The discovery of medium-sized black holes allow us to trace the history of the giant black holes in the center of galaxies.