Speaker: Prof. Chris Done (Durham University, UK)

Time: 2:00pm; June 25

Location: Middle Conf. Room; 3rd floor

Abstract: 
I will outline how the changes in energy spectra and power spectra seen in galactic black hole can be understood in the truncated disc/hot inner flow model, and how these models give us a starting point to scale up to the supermassive black holes in AGN.