The Messenger 148
Ultra-Compact Dwarf Galaxies: Dark Matter Dominated Systems? or Simple Stellar Clusters?
Padova 03 3D Spectrography 3D Spectrography: II - The tracers Morphology: distribution of each component Dynamics: kinematics via the emission or absorption.
Http://chandra.h arvard.edu/phot o/2007/m51/. Confronting Stellar Feedback Simulations with Observations of Hot Gas in Elliptical Galaxies Q. Daniel Wang,
FIGGS: The Faint Irregular Galaxy GMRT Survey Jayaram N Chengalur NCRA/TIFR Ayesha Begum I. D. Karachentsev Sambit Roychowdhury S. Kaisin, M. Sharina.
The Outermost Regions of Galactic Disks Ken Freeman RSAA, ANU MNRF Symposium 7.6.05 NGC 6946: WSRT, Tom Oosterloo.
BROWN DWARFS The coldest stars in the Universe Ngoc Phan-Bao HCM International University-Vietnam National University Image credit: JPL/NASA Workshop on.
Tiziana Di Matteo et al- Direct Cosmological Simulations of the Growth of Black Holes and Galaxies
Orange Basin Modelling
Dark energy workshop Copenhagen Aug. 2007. Why the SNLS ? Questions to be addressed: -Can the intrinsic scatter in the Hubble diagram be further reduced?
Our CMB Motion: The Local Void influence Voids Devoid of Dwarfs: Cosmology or Gastrophysics? Brent Tully Institute for Astronomy University of Hawaii.
Southwest Research Institute J.O. Parra, C.L. Hackert, Southwest Research Institute; H.A. Collier, Collier Consulting; M. Bennett, South Florida Water.