Simulations of galaxy mergers Thorsten Naab MPA, Garching Evolution of galaxies, their central black holes and their large scale environment Potsdam, September,
Classifying galaxies is hard, and different people do it different ways Except for nearby, we can only see bright galaxies I will ignore dwarf spheroidal.
Exploring the line-of-sight environment to a quasar with Gemini/GMOS. Matthew Whiting (UNSW) Rachel Webster (U. Melbourne) Paul Francis (ANU)
The Electromagnetic Spectrum 2011
Remnants of the_sagittarius_dwarf_spheroidal_galaxy_around_the_young_globular_cluster_palomar_12
When Galaxies Collide. It is not uncommon for galaxies to gravitationally interact with each other, and even collide!
Chapter 15, Galaxies G alaxies come in different size and shape. In the previous chapter, we talked about how galaxies provide an environment for the stars.
Primary-centric World-View proposes a Fractal Architecture of the Universe- A Post Copernican Conjecture. Bijay Kumar Sharma Retired Professor from NITP.
Key points: Active Galactic Nuclei: powerful energy sources in “nuclei” (very center) of some galaxies Main types: Seyferts, radio galaxies and quasars.
The two phases of massive galaxy formation Thorsten Naab MPA, Garching UCSC, August, 2010.
1 The Future of Particle Physics Steve King, University of Southampton, Masterclass, 24th March, 2009.
Announcements Test solutions are posted Pick up graded work Homework 13 is due a week from today. A spreadsheet of the data is posted on the web. No class.