HD molecules at high redshift: The absorption system at z=2.3377 towards Q 1232+082
A.V. Ivanchik, P. Petitjean, S.A. Balashev, R. Srianand, D.A., Varshalovich, C. Ledoux, and P. Noterdaeme

TL;DR
This paper analyzes H_2 and HD absorption lines in a high-redshift DLA system, deriving primordial deuterium abundance and baryon density, and suggesting infall of primordial gas onto the galaxy.
Contribution
It provides the first detailed measurement of HD and D/H ratio at high redshift, linking molecular absorption to cosmological parameters.
Findings
HD/H_2 ratio is higher than in Galactic clouds
Derived D/H ratio consistent with CMB and low-metallicity systems
Supports primordial gas infall scenario
Abstract
We present a detailed analysis of the H_2 and HD absorption lines detected in the Damped Lyman-alpha (DLA) system at z_abs=2.3377 towards the quasar Q1232+082. We show that this intervening cloud has a covering factor smaller than unity and covers only part of the QSO broad emission line region. The zero flux level has to be corrected at the position of the saturated H_2 and optically thin HD lines by about 10%. We accurately determine the Doppler parameter for HD and CI lines (b = 1.86+/-0.20 km/s). We find a ratio N(HD)/N(H_2)=(7.1 +3.7 -2.2)x10^-5 that is significantly higher than what is observed in molecular clouds of the Galaxy. Chemical models suggest that in the physical conditions prevailing in the central part of molecular clouds, deuterium and hydrogen are mostly in their molecular forms. Assuming this is true, we derive D/H = (3.6 +1.9 -1.1)x10^-5. This implies that the…
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