R-process abundances near the mass 130 peak

Details R-process abundances near the mass 130 peak R-process abundances near the mass 130 peak

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...270..746d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 270, July 15, 1983, p. 746, 747. Research supported by the Australian Resea

Astronomy and Astrophysics

Astrophysics

1

Abundance, Nuclear Fusion, Solar System, Absorption Cross Sections, Tellurium Isotopes

Scientific paper

The Kaeppeler et al. (1982) reevaluation of r-process abundances in view of new neutron-capture cross section and elemental abundance data indicates that the height of the r-process peak near mass 130 is largely determined by the r-only process nuclides Te-128 and Te-130. It is presently noted that the work of Smith, De Laeter and Rosman (1977) has not been given due consideration in the assessment of the solar system's Te abundance. These data indicate a 25 percent reduction in the height of the mass 130 peak, in agreement with s-process systematics predictions.

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