Interactions between Galaxies Galaxy Dynamics Françoise COMBES.
Clusters of galaxies The ICM, mass measurements and statistical measures of clustering.
Baryonic Dark Matter and Galaxy Formation Françoise Combes, Observatoire de Paris 29 Avril 2005.
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?
Chemistry SM-1232 Week 10 Lesson 2 Dr. Jesse Reich Assistant Professor of Chemistry Massachusetts Maritime Academy Spring 2008.
18 Dark Matter Join me on the Dark Side. 18 Goals The Universe is expanding. Will it expand forever? Depends on mass? How do we know the mass of the universe?
Unraveling HESS J1745-303 with new results from the Fermi-LAT telescope
Deep Surveys for High-z Galaxies with Hyper Suprime-Cam
Mid-Infrared Observations of Nearby Interacting/Starburst Galaxies
1 Redshifted far-IR Lines and the Cornell Caltech Atacama Telescope: CCAT A joint project of Cornell University, the California Institute of Technology.
Baryonic Dark Matter and Galaxy Formation
