A sensitive APEX and ALMA CO(1-0), CO(2-1), CO(3-2), and [CI](1-0) spectral survey of 40 local (U)LIRGs

I. Montoya Arroyave; C. Cicone; E. Makroleivaditi; A. Weiss; A. Lundgren; P. Severgnini; C. De Breuck; B. Baumschlager; A. Schimek; S. Shen; M. Aravena

doi:10.1051/0004-6361/202245046

paper

A sensitive APEX and ALMA CO(1-0), CO(2-1), CO(3-2), and [CI](1-0) spectral survey of 40 local (U)LIRGs

arXiv:2302.06629 · doi:10.1051/0004-6361/202245046

Abstract

We present a high sensitivity spectral line survey of CO(1-0), CO(2-1), CO(3-2) and [CI](1-0) in 40 local (ultra) luminous infrared galaxies ((U)LIRGs), all with previous Herschel OH119 $μ$ m observations. We use single-dish observations (PI and archival) conducted with APEX, complemented with ALMA and ACA data. We study the total emission and pay special attention to the extended low-surface brightness components. We find a tight correlation between low-J CO and [CI] line luminosities suggesting their emission arise from similar regions, at least when averaged over galactic scales. We estimate a median CO-to-H $_{2}$ conversion factor of $1.7 \pm 0.5$ M $_{⊙}$ (K km s $^{- 1}$ pc $^{2})^{- 1}$ for ULIRGs, using [CI] as an independent tracer. We derive median galaxy-integrated CO line ratios ( $r_{21}$ , $r_{31}$ and $r_{32}$ ), as well as $r_{C I C O}$ , significantly higher than normal star forming galaxies, confirming the exceptional molecular gas properties of ULIRGs. We find that $r_{21}$ and $r_{32}$ are poor tracers of CO excitation in ULIRGs, while $r_{31}$ shows a positive trend with $L_{I R}$ and SFR, and a negative trend with the H $_{2}$ gas depletion timescales ( $τ_{d e p}$ ). When studying CO line ratios as a function of gas kinematics, we find a positive relation between $r_{21}$ and $σ_{v}$ , which can be explained by CO opacity effects. We find that the linewidths of [CI] lines are ~10% narrower than CO lines, which may suggest that the low optical depth of [CI] can challenge its detection in diffuse, low-surface brightness outflows, and so its use as a tracer of CO-dark H $_{2}$ gas in these components. Finally, we find that higher $L_{A GN}$ are associated to longer $τ_{d e p}$ , consistent with the hypothesis that AGN feedback may reduce the efficiency of star formation.

arXiv commentAccepted for publication by A&A. 42 pages, 22 figures. Abstract summarised for arXiv submission

A sensitive APEX and ALMA CO(1-0), CO(2-1), CO(3-2), and [CI](1-0) spectral survey of 40 local (U)LIRGs

Abstract

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