HST/COS DETECTION OF DEUTERATED MOLECULAR HYDROGEN IN A DAMPED Lyα SYSTEM AT z = 0.18Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program #12204.

We report on the detection of deuterated molecular hydrogen, HD, at z = 0.18. HD and H2 are detected in HST/COS data of a low-metallicity (Z ∼ 0.07 Z☼) damped Lyα (DLA) system at z = 0.18562 toward QSO B0120–28, with log N(H I) = 20.50 ± 0.10. Four absorption components are clearly resolved in H2, while two components are resolved in HD; the bulk of the molecular hydrogen is associated with the components traced by HD. We find total column densities log N(HD) = 14.82 ± 0.15 and log N(H2) = 20.00 ± 0.10. This system has a high molecular fraction, f(H2) = 0.39 ± 0.10, and a low HD-to-H2 ratio, log (HD/2H2) = –5.5 ± 0.2 dex. The excitation temperature, T01 = 65 ± 2 K, in the component containing the bulk of the molecular gas is lower than in other DLAs. These properties are unlike those in other higher redshift DLA systems known to contain HD, but are consistent with what is observed in dense clouds in the Milky Way. [ABSTRACT FROM AUTHOR]