A FOURTH HI 21 cm ABSORPTION SYSTEM IN THE SIGHT LINE OF MG J0414+0534: A RECORD FOR INTERVENING ABSORBERS

作者：Tanna A^*; Curran S J; Whiting M T; Webb J K; Bignell C

来源：Astrophysical Journal Letters, 2013, 772(2): L25.

DOI：10.1088/2041-8205/772/2/L25

• galaxies: active
• galaxies: high-redshift
• galaxies: individual (MG J0414+0534)
• galaxies: ISM
• quasars: absorption lines
• radio lines: galaxies

We report the detection of a strong HI 21 cm absorption system at z = 0.5344, as well as a candidate system at z = 0.3389, in the sight line toward the z = 2.64 quasar MG J0414+0534. This, in addition to the absorption at the host redshift and the other two intervening absorbers, takes the total to four (possibly five). The previous maximum number of 21 cm absorbers detected along a single sight line is two and so we suspect that this number of gas-rich absorbers is in some way related to the very red color of the background source. Despite this, no molecular gas (through OH absorption) has yet been detected at any of the 21 cm redshifts, although, from the population of 21 cm absorbers as a whole, there is evidence for a weak correlation between the atomic line strength and the optical-near-infrared color. In either case, the fact that so many gas-rich galaxies (likely to be damped Ly alpha absorption systems) have been found along a single sight line toward a highly obscured source may have far-reaching implications for the population of faint galaxies not detected in optical surveys, a possibility which could be addressed through future wide-field absorption line surveys with the Square Kilometer Array.

• 出版日期2013-8-1
• 单位CSIRO