Detection of gamma-ray lines from interstellar 60Fe by the high resolution spectrometer SPI

Abstract

It is believed that core-collapse supernovae (CCSN), occurring at a rate about once per century, have seeded the interstellar medium with long-lived radioisotopes such as 60Fe (half-life 1.5 Myr), which can be detected by the gamma rays emitted when they beta-decay. Here we report the detection of the 60Fe decay lines at 1173 keV and 1333 keV with fluxes 3.7 +/- 1.1 x 10(-5) ph cm(-2) s(-1) per line, in spectra taken by the SPI spectrometer on board INTEGRAL during its first year. The same analysis applied to the 1809 keV line of 26Al yielded a line flux ratio 60Fe/26Al = 0.11 +/- 0.03. This supports the hypothesis that there is an extra source of 26Al in addition to CCSN.

4pp., 5 Figs., accepted by Astronomy & Astrophysics (letter), ref.'s comments included

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• Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae
• New estimates of the contribution of Wolf--Rayet stellar winds to the Galactic 26Al
• Gamma-ray line emission from OB associations and young open clusters. II. The Cygnus region
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