Linda J. Smith University College London
Three-dimensional hydrodynamical simulations of ISM pollution by type Ia and II supernovae in forming dwarf spheroidal galaxies Andrea Marcolini (Bologna.
Modelling the Stellar Populations of The Milky Way and Andromeda Collaborators: Theory:Observations: Kathryn Johnston (Columbia) Annette Ferguson (Edinburgh)
Modelling the Stellar Populations of The Milky Way and Andromeda
What can we learn from High-z Passive Galaxies ?
Stellar content of visibly obscured HII Regions
Formation & Evolution of Galaxies Stars, Gas & Dark Matter, Chemical & Dynamical Evolution
Vienna 12/04/06
The NASA/ NExScI /IPAC Star and Exoplanet Database