Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-06-19
Astronomy and Astrophysics
Astrophysics
5 pages, 3 figures, accepted by MNRAS Letters
Scientific paper
10.1111/j.1745-3933.2007.00354.x
We report the detection of 21-cm absorption at z = 0.656 towards 1622+238 (3C336). The line is very broad with a Full-Width Half Maximum (FWHM) of 235 km/s, giving a velocity integrated optical depth of 2.2 km/s. The centroid of the line is offset from that of the known damped Lyman-alpha absorption (DLA) system by 50 km/s, and if the Lyman-alpha and 21-cm absorption are due to the same gas, we derive a spin temperature of < 60 K, which would be the lowest yet in a DLA. The wide profile, which is over four times wider than that of any other DLA, supports the hypothesis that the hydrogen absorption is occurring either in the disk of a large underluminous spiral or a group of dim unidentified galaxies, associated with the single object which has been optically identified at this redshift.
Curran Stephen J.
Murphy Michael T.
Pihlstroem Ylva M.
Tzanavaris Panayiotis
Webb John K.
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