The Astrophysical Journal (Jan 2023)

The ISM in the z = 6.9 Interacting Galaxies of SPT0311-58

  • Katrina C. Litke,
  • Daniel P. Marrone,
  • Manuel Aravena,
  • Melanie Archipley,
  • Matthieu Béthermin,
  • James Burgoyne,
  • Jared Cathey,
  • Scott C. Chapman,
  • Anthony H. Gonzalez,
  • Thomas R. Greve,
  • Gayathri Gururajan,
  • Christopher C. Hayward,
  • Matthew A. Malkan,
  • Kedar A. Phadke,
  • Cassie A. Reuter,
  • Kaja M. Rotermund,
  • Justin S. Spilker,
  • Antony A. Stark,
  • Nikolaus Sulzenauer,
  • Joaquin D. Vieira,
  • David Vizgan,
  • Axel Weiß

DOI
https://doi.org/10.3847/1538-4357/acc93a
Journal volume & issue
Vol. 949, no. 2
p. 87

Abstract

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SPT0311-58, a system of two interacting galaxies in the Epoch of Reionization, exists in one of the rarest, most massive dark matter halos theoretically possible in that era. Studying the interstellar medium (ISM) in these galaxies can illuminate the process of galaxy formation in the early Universe. In this work, we explore the multiphase ISM in this system, using ALMA observations of the [C ii ] 158, [O i ] 146, [N ii ] 122, and [O iii ] 88 fine-structure lines and dust continuum. We find wide variations in line ratios between the eastern and western galaxies, as well as across the western galaxy. Continuum colors indicate that SPT0311-58 E has a higher ionization parameter ( $\mathrm{log}U\approx -2.8$ ) than SPT0311-58 W ( $\mathrm{log}U\approx -3.1$ ). The ratio of [O iii ] 88–[N ii ] 122 and the ionization parameter constraints combine to demonstrate near-solar metallicity in these objects just 800 Myr after the Big Bang.

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