A Spatially Resolved Study of Cold Dust, Molecular Gas, H II Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1
Artikel i vetenskaplig tidskrift, 2017
We present detailed studies of a z = 2.12 submillimeter galaxy, ALESS67.1, using sub-arcsecond resolution ALMA, adaptive optics-aided VLT/SINFONI, and Hubble Space Telescope (HST)/CANDELS data to investigate the kinematics and spatial distributions of dust emission (870 ?m continuum), 12CO(J = 3-2), strong optical emission lines, and visible stars. Dynamical modeling of the optical emission lines suggests that ALESS67.1 is not a pure rotating disk but a merger, consistent with the apparent tidal features revealed in the HST imaging. Our sub-arcsecond resolution data set allows us to measure half-light radii for all the tracers, and we find a factor of 4-6 smaller sizes in dust continuum compared to all the other tracers, including 12CO; also, ultraviolet (UV) and H? emission are significantly offset from the dust continuum. The spatial mismatch between the UV continuum and the cold dust and gas reservoir supports the explanation that geometrical effects are responsible for the offset of the dusty galaxy on the IRX-? diagram. Using a dynamical method we derive an , consistent with other submillimeter galaxies (SMGs) that also have resolved CO and dust measurements. Assuming a single value we also derive resolved gas and star formation rate surface densities, and find that the core region of the galaxy ( kpc) follows the trend of mergers on the Schmidt-Kennicutt relationship, whereas the outskirts ( kpc) lie on the locus of normal star-forming galaxies, suggesting different star formation efficiencies within one galaxy. Our results caution against using single size or morphology for different tracers of the star formation activity and gas content of galaxies, and therefore argue the need to use spatially resolved, multi-wavelength observations to interpret the properties of SMGs, and perhaps even for galaxies in general.
galaxies: high-redshift
cosmology: observations
galaxies: evolution
galaxies: star formation
galaxies: formation
submillimeter: galaxies
Författare
C. C. Chen
European Southern Observatory (ESO)
Durham University
J. A. Hodge
Universiteit Leiden
I. Smail
Durham University
A. M. Swinbank
Durham University
F. Walter
Max-Planck-Gesellschaft
J. M. Simpson
Academia Sinica
Gabriela Calistro Rivera
Universiteit Leiden
F. Bertoldi
Universität Bonn
W. N. Brandt
Pennsylvania State University
S. C. Chapman
Dalhousie University
E. da Cunha
Australian National University
H. Dannerbauer
Instituto de Astrofísica de Canarias
Universidad de la Laguna
C. Da Breuck
European Southern Observatory (ESO)
C. M. Harrison
European Southern Observatory (ESO)
R. J. Ivison
European Southern Observatory (ESO)
University of Edinburgh
A. Karim
Universität Bonn
Kirsten Kraiberg Knudsen
Astronomi och plasmafysik
J. L. Wardlow
Durham University
A. Weiß
Max-Planck-Gesellschaft
P. van der Werf
Universiteit Leiden
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 846 2 108Ämneskategorier
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
DOI
10.3847/1538-4357/aa863a