THE STAR FORMATION RATE EFFICIENCY of NEUTRAL ATOMIC-DOMINATED HYDROGEN GAS in the OUTSKIRTS of STAR-FORMING GALAXIES from z ∼ 1 to z ∼ 3

Marc Rafelski, Jonathan P. Gardner, Michele Fumagalli, Marcel Neeleman, Harry I. Teplitz, Norman Grogin, Anton M. Koekemoer, Claudia Scarlata

Research output: Contribution to journalArticlepeer-review

19 Scopus citations

Abstract

Current observational evidence suggests that the star formation rate (SFR) efficiency of neutral atomic hydrogen gas measured in damped Lyα systems (DLAs) at is more than 10 times lower than predicted by the Kennicutt-Schmidt (KS) relation. To understand the origin of this deficit, and to investigate possible evolution with redshift and galaxy properties, we measure the SFR efficiency of atomic gas at 1, 2, and around star-forming galaxies. We use new robust photometric redshifts in the Hubble Ultra Deep Field to create galaxy stacks in these three redshift bins, and measure the SFR efficiency by combining DLA absorber statistics with the observed rest-frame UV emission in the galaxies' outskirts. We find that the SFR efficiency of H i gas at is ∼1%-3% of that predicted by the KS relation. Contrary to simulations and models that predict a reduced SFR efficiency with decreasing metallicity and thus with increasing redshift, we find no significant evolution in the SFR efficiency with redshift. Our analysis instead suggests that the reduced SFR efficiency is driven by the low molecular content of this atomic-dominated phase, with metallicity playing a secondary effect in regulating the conversion between atomic and molecular gas. This interpretation is supported by the similarity between the observed SFR efficiency and that observed in local atomic-dominated gas, such as in the outskirts of local spiral galaxies and local dwarf galaxies.

Original languageEnglish (US)
Article number87
JournalAstrophysical Journal
Volume825
Issue number2
DOIs
StatePublished - Jul 10 2016

Bibliographical note

Funding Information:
M.F. acknowledges support by the Science and Technology Facilities Council (grant number ST/L00075X/1). Support for HST Program GO-12534 was provided by NASA through grants from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.

Publisher Copyright:
© 2016. The American Astronomical Society. All rights reserved.

Keywords

  • galaxies: evolution
  • galaxies: high-redshift
  • galaxies: photometry
  • galaxies: star formation
  • galaxies: structure
  • quasars: absorption lines

Fingerprint

Dive into the research topics of 'THE STAR FORMATION RATE EFFICIENCY of NEUTRAL ATOMIC-DOMINATED HYDROGEN GAS in the OUTSKIRTS of STAR-FORMING GALAXIES from z ∼ 1 to z ∼ 3'. Together they form a unique fingerprint.

Cite this