Centrally concentrated molecular gas driving galactic-scale ionized gas outflows in star-forming galaxies

L. M. Hogarth*, A. Saintonge, L. Cortese, T. A. Davis, S. M. Croom, J. Bland-Hawthorn, S. Brough, J. J. Bryant, B. Catinella, T. J. Fletcher, B. Groves, J. S. Lawrence, Á. R. López-Sánchez, M. S. Owers, S. N. Richards, G. W. Roberts-Borsani, E. N. Taylor, J. van de Sande, N. Scott

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

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Abstract

We perform a joint analysis of high spatial resolution molecular gas and star-formation rate (SFR) maps in main-sequence starforming galaxies experiencing galactic-scale outflows of ionized gas. Our aim is to understand the mechanism that determines which galaxies are able to launch these intense winds.We observed CO(1→0) at 1-arcsec resolution with ALMA in 16 edge-on galaxies, which also have 2-arcsec spatial-resolution optical integral field observations from the SAMI Galaxy Survey. Half the galaxies in the sample were previously identified as harbouring intense and large-scale outflows of ionized gas ('outflow types') and the rest serve as control galaxies. The data set is complemented by integrated CO(1→0) observations from the IRAM 30-m telescope to probe the total molecular gas reservoirs. We find that the galaxies powering outflows do not possess significantly different global gas fractions or star-formation efficiencies when compared with a control sample. However, the ALMA maps reveal that the molecular gas in the outflow-type galaxies is distributed more centrally than in the control galaxies. For our outflow-type objects, molecular gas and star-formation are largely confined within their inner effective radius (reff), whereas in the control sample, the distribution is more diffuse, extending far beyond reff. We infer that outflows in normal star-forming galaxies may be caused by dynamical mechanisms that drive molecular gas into their central regions, which can result in locally enhanced gas surface density and star-formation.

Original languageEnglish
Pages (from-to)3802-3820
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Volume500
Issue number3
DOIs
Publication statusPublished - 1 Jan 2021

Bibliographical note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, Volume 500, Issue 3, January 2021, Pages 3802–3820, https://doi.org/10.1093/mnras/staa3512. Copyright 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Keywords

  • galaxies: kinematics and dynamics
  • galaxies: star formation
  • submillimetre: galaxies
  • galaxies: starburst
  • galaxies: ISM
  • galaxies: evolution

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