The chemical evolution of the Milky Way: from light to heavy elements
arXiv:astro-ph/0603820 · doi:10.1063/1.2234386
Abstract
We present results for the chemical evolution of the Milky Way including predictions for elements from Deuterium to Europium. A comparison with the most accurate and recent data allows us to draw important conclusions on stellar nucleosynthesis processes as well as on mechanisms of galaxy formation.
8 pages, 7 figures, invited talk to be published in the proceedings of" Origin of Matter and Evolution of Galaxies - New Horizon of Nuclear Astrophysics and Cosmology", Ed.S.Kubono