Isotope Abundance Analyses from Stellar Spectra

Details Isotope Abundance Analyses from Stellar Spectra Isotope Abundance Analyses from Stellar Spectra

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..771...81a&link_type=abstract

ATOMIC AND MOLECULAR DATA AND THEIR APPLICATIONS: Joint Meeting of 14th Internat. Toki Conf. on Plasma Physics and Controlled Nu

Physics

Plasma Physics

Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Abundances, Chemical Composition, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

Recent chemical abundance studies, especially measurements of isotope abundance ratios, for very metal-deficient stars have provided important constraints on models of individual nucleosynthesis processes. Measurements of isotope abundances, as well as elemental abundances, from stellar spectra are briefly reviewed. Recent studies of Eu isotope ratios in metal-deficient stars, and the application to the analysis of an s-process branching are discussed.

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