Modelling the Atomic and Molecular Gas in Galaxies and Comparisons wih GASS and COLD GASS Results
A simple model to explain the high gas content of galaxy UGC 8802 Ruixiang Chang Shanghai Astronomical Observatory Collaborators: Jinliang Hou Shiyin Shen.
DM density profiles in non-extensive theory Eelco van Kampen Institute for Astro- and Particle Physics Innsbruck University In collaboration with Manfred.
The extremely high gas content of galaxy UGC8802 Chang Rui-xiang Hou Jin-liang Shen Shi-yin.
Research School of Astronomy & AstrophysicsSlide 1 SkyMapper SkyMapper and the Stromlo Southern Sky Survey Stefan Keller, Brian Schmidt, Paul Francis and.
Center for Axion and Precision Physics Strong CP-problem Axion dark-matter experiment; solar axions Proton Electric Dipole Moment experiment Muon g-2 experiment,
Introduction to Astrophysics Lecture 13: The Milky Way Galaxy.
How Do Galaxies Get Their Gas? astro-ph/0407095 Dušan Kereš University of Massachusetts Collaborators: Neal Katz, Umass David Weinberg, Ohio-State Romeel.
Nubecula Major Adric Riedel IN GLORIOUS. Outline Discovery Its place in the Local Group The LMC as a whole Gas Stars Supernovae.
A Study of Background Particles for the Implementation of a Neutron Veto into SuperCDMS Johanna-Laina Fischer Mentor: Dr. Lauren Hsu [FNAL, CDMS] September.
Raja Guhathakurta University of California Observatories / University of California Santa Cruz Email:[email protected] Cell: 408.455.3036 AAS press conference.
Final Review. Final exam Same structure: multiple choice and show- work parts Bonus questions and problems Covers chapters 15 through 18 Bring your formula.