Slide 1AGB stars in Galactic Globular Clusters – Are They Chemically Distinct to Their Fellow RGB and HB Stars? M5: SDSS Simon Campbell Slide 2 Collaborators RSAA, Mt Stromlo,…

Slide 1Significant age range in massive star cluster excluded by tight sub-giant-branch morphology Chengyuan Li Richard de Grijs Licai Deng Science lead the way. 以化成天下。…

Slide 1 Slide 2 ART and Science Formation of Globular Clusters in Hierarchical Cosmology: ART and Science Oleg Gnedin Ohio State University Slide 3 The outcome of models…

Significant age range in massive star cluster excluded by tight sub-giant-branch morphology Significant age range in massive star cluster excluded by tight sub-giant-branch…

THE LOCAL HIGH REDSHIFT UNIVERSE â THE EXTREMELY METAL POOR STARS IN THE GALACTIC HALO Why study very metal poor stars ? We can study the early epochs of the Galaxy, the…

Three-dimensional hydrodynamical simulations of ISM pollution by type Ia and II supernovae in forming dwarf spheroidal galaxies Andrea Marcolini (Bologna University) Fabrizio…

THE LOCAL HIGH REDSHIFT UNIVERSE â THE EXTREMELY METAL POOR STARS IN THE GALACTIC HALO Why study very metal poor stars ? We can study the early epochs of the Galaxy, the…

Slide 1 AGB stars in Galactic Globular Clusters – Are They Chemically Distinct to Their Fellow RGB and HB Stars? M5: SDSS Simon Campbell 1. Universitat Politecnica de Catalunya,…

Three-dimensional hydrodynamical simulations of ISM pollution by type Ia and II supernovae in forming dwarf spheroidal galaxies Andrea Marcolini (Bologna University) Fabrizio…