Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S262(5), p. 398-399, 2009
DOI: 10.1017/s1743921310003406
Full text: Unavailable
AbstractWe present extensive photometric and spectroscopic study to give a new insight in the bulge stellar population. Super-solar α/Fe and its constant value along the radial profile, in most of the galaxies, suggest that the star formation in these objects has been fast and occurred at the same time in the whole bulge.