Abundance of Iron-60 in Molecular Clouds

Details Abundance of Iron-60 in Molecular Clouds Abundance of Iron-60 in Molecular Clouds

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1676o&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1676

Computer Science

Scientific paper

A new model to explain the abundance of Iron-60 in the early solar
system is described. This model used supernova shocks to trigger the
rapid formation of the presolar molecular cloud. Computer simulations
test this model.

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