Thermal-instability-driven Turbulent Mixing in Galactic Disks. I. Effective Mixing of Metals

Research output: Contribution to journalArticle

Abstract

Observations show that radial metallicity gradients in disk galaxies are relatively shallow, if not flat, especially at large galactocentric distances and for galaxies in the high-redshift universe. Given that star formation and metal production are centrally concentrated, this requires a mechanism to redistribute metals. However, the nature of this mechanism is poorly understood, let alone quantified. To address this problem, we conduct magnetohydrodynamical simulations of a local shearing sheet of a thin, thermally unstable, gaseous disk driven by a background stellar spiral potential, including metals modeled as passive scalar fields. Contrary to what a simple α prescription for the gas disk would suggest, we find that turbulence driven by thermal instability is very efficient at mixing metals, regardless of the presence or absence of stellar spiral potentials or magnetic fields. The timescale for homogenizing randomly distributed metals is comparable to or less than the local orbital time in the disk. This implies that turbulent mixing of metals is a significant process in the history of chemical evolution of disk galaxies.

Details

Authors
  • Chao-Chin Yang
  • Mark Krumholz
External organisations
  • American Museum of Natural History
  • University of Illinois at Urbana-Champaign
Research areas and keywords

Subject classification (UKÄ) – MANDATORY

  • Astronomy, Astrophysics and Cosmology

Keywords

  • galaxies: abundances galaxies: ISM galaxies: kinematics and dynamics instabilities methods: numerical turbulence
Original languageEnglish
Article number48
JournalThe Astrophysical Journal
Volume758
Issue number1
Publication statusPublished - 2012
Publication categoryResearch
Peer-reviewedYes
Externally publishedYes