Search for supernova-produced Fe60 in a marine sediment
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
|Collections||ANU Research Publications|
|Source:||Physical Review Letters|
|01_Fitoussi_Search_for_supernova-produced_2008.pdf||326.96 kB||Adobe PDF||Request a copy|
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