Astronomy and Astrophysics – Astronomy
Scientific paper
May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.2307y&link_type=abstract
American Astronomical Society, 188th AAS Meeting, #23.07; Bulletin of the American Astronomical Society, Vol. 28, p.855
Astronomy and Astrophysics
Astronomy
Scientific paper
Heavy element abundances derived for QSO absorption line systems at 2 < z < 4 are used to predict the z dependence of [D/H] in the same systems. The scatter in the heavy element abundances, and the fact that these are actually upper limits, lead us to conclude that a constant value of [D/H] is not expected. Furthermore, the small region actually sampled in the QSO beam may prohibit the necessary averaging over a entire galaxy to see a direct correlation between astration of deuterium and production of heavy elements. These considerations may help resolve the apparent range of a factor of 5 or more found in [D/H] at 2 < z < 5 by different groups studying different systems.
Lauroesch James Thomas
Timmes Francis X.
Truran Jame. W.
York Don G.
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