Abundances and Abundance Ratios in our Galaxy and the Local Group

Eline Tolstoy
2006 Proceedings of the International Astronomical Union  
This is a review of the progress of ESO/WFI Imaging and VLT/FLAMES spectroscopy of large numbers of individual stars in nearby dwarf spheroidal galaxies primarily by the Dwarf Abundances and Radial-velocities Team (DART). These observations have allowed us to show that neither the kinematics nor the abundance nor the spatial distributions are easy to explain in a straight forward manner for these smallest galaxies. The main result is that dwarf galaxies show complex and highly specific
more » ... y specific evolutionary and metal enrichment processes, especially at ancient times. This conclusively proves that these small galaxies are not the building blocks of the larger galaxies in the Local Group.
doi:10.1017/s1743921307008162 fatcat:hhhnjwtbzvhrdlrf5zgfykwngi