Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982rspta.307...19p&link_type=abstract
(Royal Society, Discussion on the Big Bang and Element Creation, London, England, Mar. 11, 12, 1982.) Royal Society (London), Ph
Astronomy and Astrophysics
Astrophysics
78
Abundance, Astrophysics, Big Bang Cosmology, Helium Isotopes, Interstellar Matter, Light Elements, Baryons, Deuterium, Galactic Evolution, Globular Clusters, H Ii Regions, Hydrogen Isotopes, Lithium Isotopes, Main Sequence Stars, Nuclear Fusion, Solar System
Scientific paper
An attempt is made to explain current knowledge about the present abundance of H-1, D, He-3, He-4, and Li-7 in the intestellar medium and what estimates of their primordial abundances can be made when the effects of nuclear synthesis and destruction are allowed for. Estimates of present-day and primordial abundances of the relevant elements are summarized and plotted against the predicted Big-Bang values. Greatest emphasis is given to helium, with its abundance estimated for the solar neighborhood, globular clusters and field stars of the galactic halo population, and galactic and extragalactic H II regions.
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