Nucleosynthesis of Fe60 in massive stars
Astrophysics
2009-11-13 v2
Abstract
We discuss at some extent the production of Fe60 in massive stars in the range between 11 and 120 Msun both in the hydrostatic and explosive stages. We also compare the Fe60/Al26 gamma-ray line flux ratio obtained according to the present calculations to the detected value reported by INTEGRAL/SPI.
Cite
@article{arxiv.astro-ph/0512598,
title = {Nucleosynthesis of Fe60 in massive stars},
author = {M. Limongi and A. Chieffi},
journal= {arXiv preprint arXiv:astro-ph/0512598},
year = {2009}
}
Comments
8 pages, 2 figures, in proceedings of Astronomy with Radioactivities V, Clemson University, September 5-9, 2005, to appear in New Astronomy Reviews. Revised Version