Magnesium Isotopes in Halo Stars of Various Metallicities

Details Magnesium Isotopes in Halo Stars of Various Metallicities Magnesium Isotopes in Halo Stars of Various Metallicities

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984msngr..35...25b&link_type=abstract

The Messenger, No. 35, P.25, 1984

Computer Science

Scientific paper

Population II stars are very old objects, and their relative abundances can give clues on the chemical enrichment at early times. The elemental composition of stars depends on the initial mass function of the progenitor stars which enrich the gas from which they form. Some element ratios in the oldest stars are especially sensitive to the mass of the preceding stars, the so-called population 111 or population O, first generation of zero-metal stars, today disappeared.

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