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The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies

Simpson, J.M.; Smail, I.; Swinbank, A.M.; Almaini, O.; Blain, A.W.; Bremer, M.N.; Chapman, S.C.; Chen, C.-C.; Conselice, C.; Coppin, K.E.K.; Danielson, A.L.R.; Dunlop, J.S.; Edge, A.C.; Farrah, D.; Geach, J.E.; Hartley, W.G.; Ivison, R.J.; Karim, A.; Lani, C.; Ma, C.-J.; Meijerink, R.; Michalowski, M.J.; Mortlock, A.; Scott., D.; Simpson, C.J.; Spanns, M.; Thomson, A.P.; van Kampen, E.; van der Werf, P.P.

The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies Thumbnail


Authors

J.M. Simpson

O. Almaini

A.W. Blain

M.N. Bremer

S.C. Chapman

C.-C. Chen

C. Conselice

K.E.K. Coppin

A.L.R. Danielson

J.S. Dunlop

D. Farrah

J.E. Geach

W.G. Hartley

R.J. Ivison

A. Karim

C. Lani

C.-J. Ma

R. Meijerink

M.J. Michalowski

A. Mortlock

D. Scott.

C.J. Simpson

M. Spanns

A.P. Thomson

E. van Kampen

P.P. van der Werf



Abstract

We present high-resolution (0.''3) Atacama Large Millimeter Array 870 μm imaging of 52 sub-millimeter galaxies (SMGs) in the Ultra Deep Survey field to investigate the size and morphology of the sub-millimeter (sub-mm) emission on 2-10 kpc scales. We derive a median intrinsic angular size of FWHM = 0.''30 ± 0.''04 for the 23 SMGs in the sample detected at a signal-to-noise ratio (S/N) >10. Using the photometric redshifts of the SMGs we show that this corresponds to a median physical half-light diameter of 2.4 ± 0.2 kpc. A stacking analysis of the SMGs detected at S/N <10 shows they have sizes consistent with the 870 μm bright SMGs in the sample. We compare our results to the sizes of SMGs derived from other multi-wavelength studies, and show that the rest-frame ~250 μm sizes of SMGs are consistent with studies of resolved 12CO (J = 3-2 to 7-6) emission lines, but that sizes derived from 1.4 GHz imaging appear to be approximately two times larger on average, which we attribute to cosmic ray diffusion. The rest-frame optical sizes of SMGs are around four times larger than the sub-millimeter sizes, indicating that the star formation in these galaxies is compact relative to the pre-existing stellar distribution. The size of the starburst region in SMGs is consistent with the majority of the star formation occurring in a central region, a few kiloparsecs in extent, with a median star formation rate surface density of 90 ± 30 M ☉ yr–1 kpc–2, which may suggest that we are witnessing an intense period of bulge growth in these galaxies.

Journal Article Type Article
Acceptance Date Nov 15, 2014
Online Publication Date Jan 16, 2015
Publication Date Jan 20, 2015
Deposit Date Jan 30, 2015
Publicly Available Date Apr 13, 2015
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 799
Issue 1
Article Number 81
DOI https://doi.org/10.1088/0004-637x/799/1/81
Keywords Galaxies: high-redshift, Galaxies: starburst.
Public URL https://durham-repository.worktribe.com/output/1415759
Related Public URLs http://adsabs.harvard.edu/abs/2015ApJ...799...81S

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Copyright Statement
© 2015. The American Astronomical Society. All rights reserved.






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