The chemical evolution of the solar neighbourhood
Astrophysics
2016-01-27 v2
Abstract
Recent models of galactic chemical evolution account for updated evolutionary models of massive stars (with special emphasis on stellar winds) and for the effects of intermediate mass and massive binaries. The results are summarised. We also present a critical discussion on possible effects of stellar rotation on overall galactic chemical evolutionary simulations.
Cite
@article{arxiv.astro-ph/0209066,
title = {The chemical evolution of the solar neighbourhood},
author = {D. Vanbeveren and E. De Donder},
journal= {arXiv preprint arXiv:astro-ph/0209066},
year = {2016}
}
Comments
12 pages, 3 figures, Pacific Rim Conference, Xi'an, China, 11-17 July 2002