Limits on Supernova-Associated <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>Fe</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>60</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>/</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi>Al</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>26</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math> Nucleosynthesis Ratios from Accelerator Mass Spectrometry Measurements of Deep-Sea Sediments
Jenny Feige(University of Vienna), Stephan Winkler(University of Vienna), Georg Rugel(Technical University of Munich), Randolf Altmeyer(Humboldt-Universität zu Berlin), A. Wallner(Australian National University), Peter Steier(University of Vienna), Robin Golser(University of Vienna), L.K. Fifield(Australian National University), Silke Merchel(Helmholtz-Zentrum Dresden-Rossendorf), S.G. Tims(Australian National University)
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