HI Gas as Function of Environment When and where do galaxies stop accreting cool gas? How do they loose the cool gas? When do they stop forming stars?
The assembly of stellar mass during the last 10 Gyr: VVDS results B.Garilli on behalf of the VVDS consortium 1 topic, 4 approaches, concordant results.
Discovery of Galaxy Clusters Around Redshift 1
Dissecting the Red Sequence: Star Formation Histories & Mass to Light Ratios
Discovery of Galaxy Clusters Around Redshift 1 Deborah Haarsma, Calvin College @ GLCW, June 1, 2007.
Major dry-merger rate and extremely massive major dry-mergers of BCGs Deng Zugan June 31st 2008. Taiwan.
Major dry-merger rate and extremely massive major dry- mergers of BCGs Deng Zugan
HI Gas as Function of Environment
