New insights into the astrophysical r-process

Details New insights into the astrophysical r-process New insights into the astrophysical r-process

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990natur.345..491m&link_type=abstract

Nature (ISSN 0028-0836), vol. 345, June 7, 1990, p. 491-494. Research supported by DOE and NSF.

Astronomy and Astrophysics

Astrophysics

111

Abundance, Branching (Physics), Decay Rates, Neutron Decay, Nuclear Fusion, Supernovae, Astrophysics, Chemical Elements, Galactic Evolution, Solar System

Scientific paper

Elements heavier than iron are known to be made partly by rapid neutron
capture - the astrophysical r-process. New data from nuclear experiments
and astronomical observations may allow some of the proposed
astrophysical sites for the r-process to be ruled out and suggest that
these elements are mostly produced in type II supernovae.

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