The cooling-flow problem Bremsstrahlung emission ) L / n2 ) center parts cool faster. Pressure equilibrium ) mass in-flow ) density increases. Mariano Mendez - SRON The cooling-flow…

Coevolution of black holes and galaxies at high redshift David M Alexander (Durham) The growth of black holes Black Hole Accretion Disk Action: Star formation Action: AGN…

SNAP-L A wide field imager for dark energy … and more ! Jean-Paul KNEIB LAM, Marseille, France Jean-Paul KNEIB - prospective spatial PNG The SNAP-L Mission SNAP-L is a…

Slide 1 Radio Emission in Galaxies Jim Condon NRAO, Charlottesville At a meeting on “Infrared Emission, ISM, and Star Formation” in galaxies, why have a review of radio…

FMOS Science Workshop (Oxford, 22-23/06/2009) Star Formation History in Biased Regions at 0.4 z = 30 z = 5 z = 2 z = 3 z = 0 z = 1 Origin of Environmental Dependence Nature?…

The Evolution of Super-Massive Black Holes Ezequiel Treister (IfA, Hawaii) Meg Urry, Priya Natarajan (Yale) Dave Sanders (IfA) Eric Gawiser (Rutgers) Credit: ESO/NASA, the…

Dust obscured radio-quiet quasars at high redshifts Mark Lacy, NAASC/NRAO Andreea Petric (SSC), Susan Ridgway (CTIO), Tanya Urrutia (SSC), Anna Sajina (Haverford), Alejo…

Active Galaxies and Related Objects What are Active Galaxies? Active galaxies have an energy source beyond what can be attributed to stars. The energy is believed to originate…

Assigning a distance by redshift The Hubble law lets us use a simple spectrum of a galaxy to figure out where it is along the line-of-sight. Higher redshifts indeed go with…

Unveiling HIZOAJ0836-43 The SED of the nearby, HI-massive, LIRG HIZOA J0836-43: from the NIR to the radio domain Renée C. Kraan-Korteweg Astronomy Department Centre for…