Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 0346–52
Abstract

With ΣSFR∼ 4200Myr−1kpc−2, SPT 0346–52 (z= 5.7) is the most intensely star-forming galaxy discovered by the South Pole Telescope. In this paper, we expand on previous spatially resolved studies, using ALMA observations of dust continuum, [Nii] 205μm, [Cii] 158μm, [Oi] 146μm, and undetected [Nii] 122μm and [Oi] 63μm emission to study the multiphase interstellar medium (ISM) in SPT 0346–52. We use pixelated, visibility-based lens modeling to reconstruct the source-plane emission. We also model the source-plane emission using the photoionization codecloudyand find a supersolar metallicity system. We calculateTdust= 48.3 K andλpeak= 80μm and see line deficits in all five lines. The ionized gas is less dense than comparable galaxies, withne< 32 cm−3, while ∼20% of the [Cii] 158μm emission originates from the ionized phase of the ISM. We also calculate the masses of several phases of the ISM. We find that molecular gas dominates the mass of the ISM in SPT 0346–52, with the molecular gas mass ∼4× higher than the neutral atomic gas mass and ∼100× higher than the ionized gas mass.

Authors:
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Award ID(s):
Publication Date:
NSF-PAR ID:
10365012
Journal Name:
The Astrophysical Journal
Volume:
928
Issue:
2
Page Range or eLocation-ID:
Article No. 179
ISSN:
0004-637X
Publisher:
DOI PREFIX: 10.3847
National Science Foundation
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