H I 21 cm absorption at z 2.347 towards PKS B0438-436

Kanekar, N. ; Subrahmanyan, R. ; Ellison, S. L. ; Lane, W. M. ; Chengalur, J. N. (2006) H I 21 cm absorption at z 2.347 towards PKS B0438-436 Monthly Notices of the Royal Astronomical Society, 370 (1). L46-L50. ISSN 0035-8711

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Official URL: http://doi.org/10.1111/j.1745-3933.2006.00186.x

Related URL: http://dx.doi.org/10.1111/j.1745-3933.2006.00186.x

Abstract

We report the detection of redshifted H I 21-cm absorption in the z∼ 2.347 damped Lyman a absorber (DLA) towards PKS B0438-436 with the Green Bank Telescope. This is the second-highest redshift at which 21-cm absorption has been detected in a DLA. The absorption extends over ∼60 km s-1 and has two distinct components, at z= 2.347 477(12) and z= 2.347 869(20). A similar velocity structure is seen in optical metal lines, although the peak absorption here is offset by ∼11 km s-1 from the peak in the 21-cm line. We obtain a high spin temperature Ts∼ (886 ± 248) × (f/0.58) K, using a covering factor estimated from 2.3-GHz very long baseline interferometry data. However, the current data cannot rule out a low spin temperature. The non-detection of CO 3-2 absorption places the upper limit NCO < 3.8 × 1015 (Tx/10) cm-2 on the CO column density.

Item Type:Article
Source:Copyright of this article belongs to Oxford University Press.
Keywords:Galaxies: High-Redshift; Galaxies: ISM; Radio Lines: Galaxies.
ID Code:118116
Deposited On:14 May 2021 06:21
Last Modified:14 May 2021 06:21

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