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Nucleosynthesis of 60Fe in massive stars

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Oct 2006Embargo end date: 01 Dec 2005 English Publisher:Elsevier BVJournal:New Astronomy Reviews, volume 50, pages 474-476 (issn: 1387-6473, Copyright policy )
Authors: Limongi, M.; Chieffi, A.;

doi: 10.1016/j.newar.2006.06.005 , 10.48550/arxiv.astro-ph/0512598

arXiv: astro-ph/0512598

Nucleosynthesis of 60Fe in massive stars

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.

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

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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    popularity
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    		 Top 10%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
19
Top 10%
Average
Average
Green
bronze