Search for supernova-produced Fe60 in a marine sediment
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Date
Authors
Fitoussi, C.
Raisbeck, G.M.
Knie, K.
Korschinek, Gunther
Faestermann, T.
Goriely, S
Lunney, D.
Poutivtsev, M.
Rugel, G.
Waelbroeck, Claire
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American Physical Society
Abstract
An Fe60 peak in a deep-sea FeMn crust has been interpreted as due to the signature left by the ejecta of a supernova explosion close to the solar system 2.8±0.4Myr ago. In an attempt to confirm this interpretation with better time resolution and obtain a
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Source
Physical Review Letters
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Restricted until
2037-12-31