The Messenger 147
AGB stars in Galactic Globular Clusters – Are They Chemically Distinct to Their Fellow RGB and HB Stars? M5: SDSS Simon Campbell.
Significant age range in massive star cluster excluded by tight sub-giant-branch morphology Chengyuan Li Richard de Grijs Licai Deng Science lead the way.
ART and Science Formation of Globular Clusters in Hierarchical Cosmology: ART and Science Oleg Gnedin Ohio State University.
Significant age range in massive star cluster excluded by tight sub-giant-branch morphology
1 THE LOCAL HIGH REDSHIFT UNIVERSE – THE EXTREMELY METAL POOR STARS IN THE GALACTIC HALO Why study very metal poor stars ? We can study the early epochs.
Three-dimensional hydrodynamical simulations of ISM pollution by type Ia and II supernovae in forming dwarf spheroidal galaxies Andrea Marcolini (Bologna.
How Many SN Contribute to an EMP Star’s Chemical Inventory ?
AGB stars in Galactic Globular Clusters – Are They Chemically Distinct to Their Fellow RGB and HB Stars?
Vienna 12/04/06
