SPI observations of the diffuse60Fe emission in the Galaxy

2007/04/30 by W. Wang, M. J. Harris, R. Diehl +13 · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Gamma-ray bursts and supernovae #astro-ph #nucl-ex #nucl-th

paper · pdf · doi:10.1051/0004-6361:20066982

published as Astron.Astrophys.469:1005,2007 · 10 pages, 7 figures, 2 tables, A&A in press

arxiv created 2007/04/30 · openalex publication_date 2007/05/10 · arxiv updated 2009/12/01 · openalex created_date 2019/06/27 · openalex updated_date 2026/07/31

Abstract

Aims.Gamma-ray line emission from radioactive decay of 60Fe provides constraints on nucleosynthesis in massive stars and supernovae.

Citations

• Detection of γ-ray lines from interstellar \mathsf⁶⁰Fe by the high resolution spectrometer SPI

Cited by

• New Measurement of theFe<mml:mprescripts/><mml:none/>60Half-Life