Slide 1Image credit: NASA, ESA and A. Evans (Stony Brook University, New York) Probing the evolution of merger remnants via formation of cold molecular gas disks Junko Ueda…
Slide 1 Once we know the surface brightness profile of a galaxy, we can integrate it from 0 to to the total integrated apparent magnitude of a galaxy in a given band:…
The connection between galaxies and quasar absorption lines Lise Christensen Quasar absorption lines DLA LLS Lya forest Metal lines Types of systems Charlton, 2000 Lya forest…
Once we know the surface brightness profile of a galaxy, we can integrate it from 0 to to the total integrated apparent magnitude of a galaxy in a given band: ( for a…
Galaxies GALAXIES Do Now Take a sheet of paper and answer the following questions. What are two kinds of visible light telescopes scientists use to gather information from…
Estudio de Cúmulos de Galaxias en el Sloan Digital Sky Survey “Nature and Descendants of Sub-mm and Lyman-break Galaxies in Lambda-CDM” Juan Esteban González Obergurgl,…
Estudio de Cúmulos de Galaxias en el Sloan Digital Sky Survey “Nature and Descendants of Sub-mm and Lyman-break Galaxies in Lambda-CDM” Juan Esteban González Obergurgl,…