Big-Bang vs. Galactic Origin of Elements in Metal-Deficient Stars

Details Big-Bang vs. Galactic Origin of Elements in Metal-Deficient Stars Big-Bang vs. Galactic Origin of Elements in Metal-Deficient Stars

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..572k&link_type=abstract

Nuclear Physics A, v. 621, p. 572-575.

Physics

Nuclear Physics

Scientific paper

Accretion of interstellar material onto the metal-deficient halo stars that plunge through the disk is expected to mask the earlier production of the light elements in the big-bang nucleosynthesis. We propose a method to distinguish the primordial yield from that accreted in the secondary intragalactic motion of the stars by the use of heavy r- and s-process elements in these stars.

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