The chemical evolution of the Milky Way: from light to heavy elements
Astrophysics
2009-11-11 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/0603820,
title = {The chemical evolution of the Milky Way: from light to heavy elements},
author = {Francesca Matteucci},
journal= {arXiv preprint arXiv:astro-ph/0603820},
year = {2009}
}
Comments
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