Planck 's Dusty GEMS: VII. Atomic carbon and molecular gas in dusty starburst galaxies at z = 2 to 4
Artikel i vetenskaplig tidskrift, 2019

The bright 3 P 1 - 3 P 0 ([CI] 1-0) and 3 P 2 - 3 P 1 ([CI] 2-1) lines of atomic carbon are becoming more and more widely employed as tracers of the cold neutral gas in high-redshift galaxies. Here we present observations of these lines in the 11 galaxies of the set of Planck's Dusty GEMS, the brightest gravitationally lensed galaxies on the extragalactic submillimeter sky probed by the Planck satellite. We have [CI] 1-0 and [CI] 2-1 measurements for seven and eight of these galaxies, respectively, including four galaxies where both lines have been measured. We use our observations to constrain the gas excitation mechanism, excitation temperatures, optical depths, atomic carbon and molecular gas masses, and carbon abundances. Ratios of L CI /L FIR are similar to those found in the local universe, and suggest that the total cooling budget through atomic carbon has not significantly changed in the last 12 Gyr. Both lines are optically thin and trace 1 - 6 × 10 7 M of atomic carbon. Carbon abundances, X CI , are between 2.5 and 4 × 10 -5 , for an ultra-luminous infrared galaxy (ULIRG) CO-to-H 2 conversion factor of α CO = 0.8 M / [K km s -1 pc 2 ]. Ratios of molecular gas masses derived from [CI] 1-0 and CO agree within the measurement uncertainties for five galaxies, and agree to better than a factor of two for another two with [CI] 1-0 measurements, after carefully taking CO excitation into account. This does not support the idea that intense, high-redshift starburst galaxies host large quantities of "CO-dark" gas. These results support the common assumptions underlying most molecular gas mass estimates made for massive, dusty, high-redshift starburst galaxies, although the good agreement between the masses obtained with both tracers cannot be taken as independent confirmation of either α CO or X CI .

Galaxies: formation

Galaxies: abundances

Galaxies: high-redshift

Galaxies: starburst

Författare

N. P.H. Nesvadba

Université Paris-Sud

R. Canameras

Niels Bohr Institute

R. Kneissl

Atacama Large Millimeter-submillimeter Array (ALMA)

European Southern Observatory Santiago

Sabine König

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

C. Yang

European Southern Observatory Santiago

E. Le Floc'H

Université Paris Diderot

A.A. Omont

Institut d 'Astrophysique de Paris

Douglas Scott

University of British Columbia (UBC)

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 624 A23

Ämneskategorier

Astronomi, astrofysik och kosmologi

Atom- och molekylfysik och optik

Den kondenserade materiens fysik

DOI

10.1051/0004-6361/201833777

Mer information

Senast uppdaterat

2019-05-06