Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South : near-infrared morphologies and stellar sizes.

Chen, C.-C. and Smail, I. and Swinbank, A. M. and Simpson, J. M. and Ma, C.-J. and Alexander, D. M. and Biggs, A. D. and Brandt, W. N. and Chapman, S. C. and Coppin, K. E. K. and Danielson, A. L. R. and Dannerbauer, H. and Edge, A. C. and Greve, T. R. and Ivison, R. J. and Karim, A. and Menten, K. M. and Schinnerer, E. and Walter, F. and Wardlow, J. L. and Weiss, A. and van der Werf, P. P. (2015) 'An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South : near-infrared morphologies and stellar sizes.', Astrophysical journal., 799 (2). p. 194.

Abstract

We analyze Hubble Space Telescope WFC3/H 160-band observations of a sample of 48 Atacama Large Millimeter/submillimeter Array detected submillimeter galaxies (SMGs) in the Extended Chandra Deep Field South field, to study their stellar morphologies and sizes. We detect 79% ± 17% of the SMGs in the H 160-band imaging with a median sensitivity of 27.8 mag, and most (80%) of the nondetections are SMGs with 870 μm fluxes of S 870 < 3 mJy. With a surface brightness limit of μ H ~ 26 mag arcsec–2, we find that 82% ± 9% of the H 160-band-detected SMGs at z = 1-3 appear to have disturbed morphologies, meaning they are visually classified as either irregulars or interacting systems, or both. By determining a Sérsic fit to the H 160 surface brightness profiles, we derive a median Sérsic index of n = 1.2 ± 0.3 and a median half-light radius of re = 4.4$^{+1.1}_{-0.5}$ kpc for our SMGs at z = 1-3. We also find significant displacements between the positions of the H 160 component and 870 μm emission in these systems, suggesting that the dusty starburst regions and less-obscured stellar distribution are not colocated. We find significant differences in the sizes and the Sérsic index between our z = 2-3 SMGs and z ~ 2 quiescent galaxies, suggesting that a major transformation of the stellar light profile is needed in the quenching processes if SMGs are progenitors of the red-and-dead z ~ 2 galaxies. Given the short-lived nature of SMGs, we postulate that the majority of the z = 2-3 SMGs with S 870 gsim 2 mJy are early/mid-stage major mergers.

Item Type:Article
Keywords:Cosmology: observations, Galaxies: formation, Galaxies: starburst, Submillimeter: galaxies.
Full text:(VoR) Version of Record
Download PDF
(5998Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1088/0004-637X/799/2/194
Publisher statement:© 2015. The American Astronomical Society. All rights reserved.
Date accepted:No date available
Date deposited:13 April 2015
Date of first online publication:February 2015
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar