Recent Talks

2- More on isochrones

- bolometric corrections and Teff-color relations

- populating isochrones, and the IMF

- simulating star clusters

- simulating apparent and detached binaries

- simulating interacting binaries

2- Stellar orbits and dynamical models

- orbits in various potentials, Jeans Thm, DF models, Schwarzschild, M2M

2- The thin disk.

- observational issues with the star formation history and the dynamical evolution of the thin disk.

- continuing gas accretion

- theoretical ideas about the formation and evolution of the thin disk.

2- Poisson solvers

- trees

- fixed and adaptive grids

- parallelization

1-  Overview of the structure of our Galaxy in the context of other galaxies

- the basic components

- dark matter properties

- general ideas about galaxy assembly

1- The basics

- overview of stellar evolution as a function of mass and metallicity

- from evolutionary tracks to isochrones

- quick overview of chemical changes at the stellar surface

1- Fundamental stellar dynamics

- relaxation, collisionless dynamics

- distribution functions, Jeans eqs, etc.

1- The use and abuse of N-body codes

- relaxation in spheres and disks,  collective enhancement

- code structure, block time steps

It is now clear that supermassive black holes (M>1e6 Msun) live in the center of most (all) galaxies, including our own Milky Way. Furthermore, the energy released during the growth of this black hole is a critical ingredient in understanding galaxy formation and evolution. In this talk, I will show what we know about how, when and where these supermassive black holes are acquiring their masses. In particular, I will focus on the effects of obscuration, as it is now clear that the majority of this black hole growth is hidden from our view by large amounts of gas and dust. I will present statistical evidence suggesting that while most nuclear activity is triggered by internal secular processes, the most violent episodes are linked to major galaxy mergers. Finally, I will show how future data obtained combining observations with the ALMA radio telescope and the NuSTAR X-ray observatory will allow us to understand the physical details of the connection between black hole growth and galaxy evolution.

In the past few years, a series of discoveries have been made of objects which appear to be accreting stellar mass black holes in globular clusters -- both in the Milky Way and in other nearby galaxies. I will discuss why the theoretical work which suggested that such objects would be unlikely to exist, the observations showing they do exist, some of the unusual aspects of some of the individual sources, and the new theoretical framework for producing them.