Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201l..51o&link_type=abstract
Astrophysical Journal, vol. 201, Oct. 15, 1975, pt. 2, p. L51-54.
Astronomy and Astrophysics
Astrophysics
25
Abundance, Cosmology, Deuterium, Galactic Evolution, Astronomical Models, Big Bang Cosmology, H Ii Regions, Line Spectra, Radiative Recombination
Scientific paper
If deuterium is made primarily in stars, then according to current models of galactic evolution it should have a higher abundance in the metal-rich parts of the Galaxy. If it is produced only in the initial big bang, then astration causes a decrease in D abundance with increasing metal abundance z. Since the sign of the galactic metal abundance gradient is known to be negative, it is proposed that a determination of the sign of the deuterium abundance gradient would indicate the probable origin of this isotope. In particular it appears possible that the ratio of the radio recombination line strengths (D/H) from dense H II regions might be measurable with realizable equipment and determine, relatively unambiguously, the ratio of abundances in various parts of the Galaxy.
Ostriker Jeremiah P.
Tinsley Beatrice M.
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