Slide 1 Martin Bureau, Oxford University The Tully-Fisher Relation: Across Morphological Types and Redshift Martin Bureau, Oxford University Plans: Galaxy formation, scaling…

MATISSE - Rencontre projet Fizeau Nov. 2010 Schedule Dec 2010 PDR June 2011 OFDR Dec 2011 FDR Mar 2013 N Cold Optics Apr 2013 N Cryostat Jun 2013 Integration N Cold Optics,…

MATISSE - Rencontre projet Fizeau Nov. 2010 Schedule Dec 2010 PDR June 2011 OFDR Dec 2011 FDR Mar 2013 N Cold Optics Apr 2013 N Cryostat Jun 2013 Integration N Cold Optics,…

How do Black Hole Accretion Disks Radiate? Shane Davis UCSB Standard Accretion Picture Issues Addressed in This Talk How does the release of gravitational binding energy…

High Resolution Mid-Infrared Imaging of Dusty Circumstellar Structure around Evolved Stars with the MMT Adaptive Optics System B.A. Biller, L.M. Close, A. Li, J.H. Bieging,…

How do Black Hole Accretion Disks Radiate? Shane Davis UCSB Standard Accretion Picture Issues Addressed in This Talk How does the release of gravitational binding energy…