Almacal – VI. Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers
Artikel i vetenskaplig tidskrift, 2019

We are just starting to understand the physical processes driving the dramatic change in cosmic star formation rate between z ∼ 2 and the present day. A quantity directly linked to star formation is the molecular gas density, which should be measured through independent methods to explore variations due to cosmic variance and systematic uncertainties. We use intervening CO absorption lines in the spectra of mm-bright background sources to provide a census of the molecular gas mass density of the Universe. The data used in this work are taken from ALMACAL, a wide and deep survey utilizing the ALMA calibrator archive. While we report multiple Galactic absorption lines and one intrinsic absorber, no extragalactic intervening molecular absorbers are detected. However, due to the large redshift path surveyed (z = 182), we provide constraints on the molecular column density distribution function beyond z ∼ 0. In addition, we probe column densities of N(H2) > 1016 atoms cm−2, 5 orders of magnitude lower than in previous studies. We use the cosmological hydrodynamical simulation IllustrisTNG to show that our upper limits of ρ(H2) 108.3 M Mpc−3 at 0 < z ≤ 1.7 already provide new constraints on current theoretical predictions of the cold molecular phase of the gas. These results are in agreement with recent CO emission-line surveys and are complementary to those studies. The combined constraints indicate that the present decrease of the cosmic star formation rate history is consistent with an increasing depletion of molecular gas in galaxies compared to z ∼ 2.

Galaxies: formation

Galaxies: evolution

Quasars: absorption lines

ISM: molecules

Författare

Anne Klitsch

European Southern Observatory (ESO)

Durham University

Céline Péroux

Laboratoire d'Astrophysique de Marseille

European Southern Observatory (ESO)

M. A. Zwaan

European Southern Observatory (ESO)

I. Smail

Durham University

Dylan Nelson

Max-Planck-Gesellschaft

Gergö Popping

Max-Planck-Gesellschaft

C. C. Chen

European Southern Observatory (ESO)

Benedikt Diemer

Harvard-Smithsonian Center for Astrophysics

R. J. Ivison

European Southern Observatory (ESO)

University of Edinburgh

James R. Allison

University of Oxford

Sebastien Muller

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Onsala rymdobservatorium, Observationssupport

A. Mark Swinbank

Durham University

Aleksandra Hamanowicz

European Southern Observatory (ESO)

A. D. Biggs

European Southern Observatory (ESO)

Rajeshwari Dutta

European Southern Observatory (ESO)

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 490 1 1220-1230

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1093/mnras/stz2660

Mer information

Senast uppdaterat

2019-12-02