Skip to main content

Research Repository

Advanced Search

Cosmic evolution of the atomic and molecular gas contents of galaxies

Lagos, C.D.P.; Baugh, C.M.; Lacey, C.G.; Benson, A.J.; Kim, H.-S.; Power, C.

Cosmic evolution of the atomic and molecular gas contents of galaxies Thumbnail


Authors

C.D.P. Lagos

A.J. Benson

H.-S. Kim

C. Power



Abstract

We study the evolution of the cold gas content of galaxies by splitting the interstellar medium into its atomic and molecular hydrogen components, using the galaxy formation model GALFORM in the Λ cold dark matter framework. We calculate the molecular-to-atomic hydrogen mass ratio, H2/H I, in each galaxy using two different approaches, the pressure-based empirical relation of Blitz & Rosolowsky and the theoretical model of Krumholz, McKeee & Tumlinson, and apply them to consistently calculate the star formation rates of galaxies. We find that the model based on the Blitz & Rosolowsky law predicts an H I mass function, 12CO (1–0) luminosity function, correlations between H2/H I and stellar and cold gas mass, and infrared–12CO molecule luminosity relation in good agreement with local and high-redshift observations. The H I mass function evolves weakly with redshift, with the number density of high-mass galaxies decreasing with increasing redshift. In the case of the H2 mass function, the number density of massive galaxies increases strongly from z= 0 to 2, followed by weak evolution up to z= 4. We also find that H2/H I of galaxies is strongly dependent on stellar and cold gas mass, and also on redshift. The slopes of the correlations between H2/H I and stellar and cold gas mass hardly evolve, but the normalization increases by up to two orders of magnitude from z= 0 to 8. The strong evolution in the H2 mass function and H2/H I is primarily due to the evolution in the sizes of galaxies and, secondarily, in the gas fractions. The predicted cosmic density evolution of H I agrees with the observed evolution inferred from damped Lyα systems, and is always dominated by the H I content of low- and intermediate-mass haloes. We find that previous theoretical studies have largely overestimated the redshift evolution of the global H2/H I due to limited resolution. We predict a maximum of Graphic at z≈ 3.5.

Citation

Lagos, C., Baugh, C., Lacey, C., Benson, A., Kim, H., & Power, C. (2011). Cosmic evolution of the atomic and molecular gas contents of galaxies. Monthly Notices of the Royal Astronomical Society, 418(3), 1649-1667. https://doi.org/10.1111/j.1365-2966.2011.19583.x

Journal Article Type Article
Publication Date Dec 11, 2011
Deposit Date Jan 31, 2012
Publicly Available Date Mar 29, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 418
Issue 3
Pages 1649-1667
DOI https://doi.org/10.1111/j.1365-2966.2011.19583.x
Keywords Stars: formation, Galaxies: evolution, Galaxies: formation, Galaxies: ISM.

Files

Published Journal Article (1.2 Mb)
PDF

Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





You might also like



Downloadable Citations