Abundances of metals in Population II stars

Details Abundances of metals in Population II stars Abundances of metals in Population II stars

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mmsai..50..121s&link_type=abstract

(Workshop on Chemical Inhomogeneities in the Galaxy, Frascati, Italy, May 29-June 2, 1978.) Società Astronomica Italiana, Memori

Astronomy and Astrophysics

Astrophysics

Abundance, Aluminum 27, Astronomical Spectroscopy, Metals, Stars, Astrophysics, Atomic Spectra

Scientific paper

Peterson (1978) has claimed that aluminum-27 is overdeficient in very-metal-poor stars. In an effort to examine Peterson's results, the present study involved the measurement of aluminum lines in the metal-poor star HD 184711. The present results disagree with those of Peterson. An attempt is made to explain this discrepancy by a gravitational sorting mechanism or by the presence of systematic errors.

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