Evidence for a_complex_enrichment_history_of_the_stream_from_fairall_9_sightline
Ultraviolet morphology and_unobscured_uv_star_formation_rates_of_clash_brighest_cluster_galaxies
New tales of molecular gas in galaxies: (not so) near and far Jeff Wagg Max-Planck/NRAO Fellow NRAO – Socorro NRAO postdoc symposium Socorro April 29,
John Salzer, Nyla Tresser, Samantha Stevenson & Hart Webb (Wesleyan University) Jessica Rosenberg (Harvard/Smithsonian CfA) Optical Properties of the HI-selected.
The Origins and Ionization Mechanisms of Warm Filaments in Cool Core Clusters Michael McDonald Postdoctoral Associate - MIT Kavli Institute In collaboration.
Active Galaxies A Short Survey. All Galaxies are active to some extent: For "normal" galaxies, we can think of the total energy output as the sum of stellar.
Formation of Globular Clusters in CDM Cosmology
Galaxies. Hubble’s Galaxy Classification American astronomer Edwin Hubble was the first to categorize galaxies in a comprehensive way. His observations.
Overview of Gas Flows: Observational Ken Freeman ANU, Canberra
