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Molecular gas in a z ∼ 2.5 triply-imaged, sub-mJy submillimetre galaxy typical of the cosmic far-infrared background

Kneib, J.-P.; Neri, R.; Smail, I.; Blain, A.; Sheth, K.; van der Werf, P.; Knudsen, K.K.

Molecular gas in a z ∼ 2.5 triply-imaged, sub-mJy submillimetre galaxy typical of the cosmic far-infrared background Thumbnail


Authors

J.-P. Kneib

R. Neri

A. Blain

K. Sheth

P. van der Werf

K.K. Knudsen



Abstract

We present the results of observations from the Plateau de Bure IRAM interferometric array of the submillimetre (submm) galaxy SMMJ16359+6612 lying at z = 2.516 behind the core of the massive cluster A2218. The foreground gravitational lens produces three images with a total magnification of 45 of this faint submm galaxy, which has an intrinsic submm flux of just f850 μm = 0.8 mJy – placing it below the confusion limit of blank-field surveys. The substantial magnification provides a rare opportunity to probe the nature of a distant sub-mJy submm-selected galaxy, part of the population which produces the bulk of the cosmic far-infrared background at submm wavelengths. Our observations detect the CO(3–2) line in all three images, as well as the CO(7–6) line and the dust continuum at 1.3 mm for the brightest image but only at a 3σ level. The velocity profile of the CO(3–2) line displays a double-peak profile which is well fit by two Gaussians with FWHM of 220 km s−1 and separated by 280 km s−1. We estimate the dynamical mass of the system to be ∼1.5 × 1010 M_ and an H2 gas mass of 4.5 × 109 M_. We identify a spatial offset of ∼1__ between the two CO(3–2) velocity components, again benefiting from the magnification due to the foreground lens, modeling of which indicates that the offset corresponds to just ∼3 kpc in projection at z = 2.516. The spatial and velocity properties of these two components are closely related to features detected in previously published Hα spectroscopy. We propose that this source is a compact merger of two typical Lyman-break galaxies with a maximal separation between the two nuclei of about 3 kpc, although a dusty disk explanation is not excluded. This system is much less luminous and massive than other high-redshift submillimetre galaxies studied to date, but it bears a close similarity to similarly luminous, dusty starburst resulting from lower-mass mergers in the local Universe.

Citation

Kneib, J., Neri, R., Smail, I., Blain, A., Sheth, K., van der Werf, P., & Knudsen, K. (2005). Molecular gas in a z ∼ 2.5 triply-imaged, sub-mJy submillimetre galaxy typical of the cosmic far-infrared background. Astronomy & Astrophysics, 434(3), 819-825. https://doi.org/10.1051/0004-6361%3A20042034

Journal Article Type Article
Publication Date May 1, 2005
Deposit Date May 28, 2013
Publicly Available Date Jun 14, 2013
Journal Astronomy and astrophysics.
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 434
Issue 3
Pages 819-825
DOI https://doi.org/10.1051/0004-6361%3A20042034
Keywords Gravitational lensing, Cosmology, Observations, Galaxies, Clusters, A2219, High-redshift, Infrared, SMM J16359+6612.

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Copyright Statement
Reproduced with permission from Astronomy & Astrophysics, © ESO





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