Sub-kiloparsec imaging of cool molecular gas in two strongly lensed dusty, star-forming galaxies

J. S. Spilker, M. Aravena, D. P. Marrone, M. B�thermin, M. S. Bothwell, J. E. Carlstrom, S. C. Chapman, J. D. Collier, C. De Breuck, C. D. Fassnacht, T. Galvin, A. H. Gonzalez, J. Gonz�lez-L�pez, K. Grieve, Y. Hezaveh, J. Ma, M. Malkan, A. O'Brien, K. M. Rotermund, M. StrandetJ. D. Vieira, A. Weiss, G. F. Wong

Research output: Contribution to journalArticlepeer-review

Abstract

We present spatially resolved imaging obtained with the Australia Telescope Compact Array (ATCA) of three CO lines in two high-redshift gravitationally lensed dusty star-forming galaxies, discovered by the South Pole Telescope. Strong lensing allows us to probe the structure and dynamics of the molecular gas in these two objects, at z = 2.78 and z = 5.66, with effective source-plane resolution of less than 1 kpc. We model the lensed emission from multiple CO transitions and the dust continuum in a consistent manner, finding that the cold molecular gas as traced by low-J CO always has a larger half-light radius than the 870 μm dust continuum emission. This size difference leads to up to 50% differences in the magnification factor for the cold gas compared to dust. In the z = 2.78 galaxy, these CO observations confirm that the background source is undergoing a major merger, while the velocity field of the other source is more complex. We use the ATCA CO observations and comparable resolution Atacama Large Millimeter/submillimeter Array dust continuum imaging of the same objects to constrain the CO-H2 conversion factor with three different procedures, finding good agreement between the methods and values consistent with those found for rapidly star-forming systems. We discuss these galaxies in the context of the star formation - gas mass surface density relation, noting that the change in emitting area with observed CO transition must be accounted for when comparing high-redshift galaxies to their lower redshift counterparts.

Original languageEnglish (US)
Article number124
JournalAstrophysical Journal
Volume811
Issue number2
DOIs
StatePublished - Oct 1 2015

Keywords

  • galaxies: high-redshift
  • galaxies: ISM
  • galaxies: star formation
  • ISM: molecules

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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