Nucleosynthesis of Fe60 in massive stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages, 2 figures, in proceedings of Astronomy with Radioactivities V, Clemson University, September 5-9, 2005, to appear in

Scientific paper

10.1016/j.newar.2006.06.005

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.

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