Slide 1Interactions between Galaxies Galaxy Dynamics Françoise COMBES Slide 2 2 NGC 2207 and IC 2163– Hubble image Slide 3 3 Arp 188 Slide 4 4 Arp 295 White contours:…

Slide 1 Slide 2 General Relativity is a surprisingly good fit for grade-9 Astronomy. It explains and gives depth to many standard topics like.... What causes orbits? What…

Slide 1Xiaohu Yang Shanghai Astronomical Observatory Partner group of MPA Collaborators: Yu Wang (SHAO), H.J. Mo (UMass), F.C. van den Bosch (MPIA), Neal Katz (UMass), A.…

Nubecula Major Adric Riedel Outline Basic Facts Discovery Morphology Its place in the Local Group Relation to the Small Magellanic Clouds As compared to other galaxies The…

Radio Jet Disruption in Cooling Cores OR, can radio jets solve the cooling core problem? OR, how do cooling cores disrupt radio jets? What is a cooling core? The old picture:…

Galaxy Collisions Top left is an image of the Cartwheel galaxy. The ring of young stars was likely created as a smaller galaxy passed through the disk of the larger one.…

Studying the gas, dust, and star formation in the first galaxies at cm and mm wavelengths Chris Carilli, KIAA-PKU reionization workshop, July 2008 QSO host galaxies at z…

Studying the gas, dust, and star formation in the first galaxies at cm and mm wavelengths Chris Carilli, KIAA-PKU reionization workshop, July 2008 QSO host galaxies at z…

The Lyman- halo of B2 0902+34: Evidence for infall of extended HI Joshua Adams & Gary Hill University of Texas, Austin Department of Astronomy 3D2008 ESO Workshop…

Obesity in the Universe: How Did Early Type Galaxies Become so Fat? Richard Ellis & Drew Newman (Caltech) CIFAR April 6th 2012 Bimodal Galaxy Distribution Bell et al.…