Disc formation and the origin of clumpy galaxies at high redshift

Oscar Agertz, Romain Teyssier, Ben Moore

Research output: Contribution to journalLetterpeer-review

216 Scopus citations

Abstract

Observations of high-redshift galaxies have revealed a multitude of large clumpy rapidly star-forming galaxies. Their formation scenario and their link to present-day spirals are still unknown. In this Letter, we perform adaptive mesh refinement simulations of disc formation in a cosmological context that are unrivalled in terms of mass and spatial resolution. We find that the so-called 'chain-galaxies' and 'clump-clusters' are a natural outcome of early epochs of enhanced gas accretion from cold dense streams as well as tidally and ram-pressured stripped material from minor mergers and satellites. Through interaction with the hot halo gas, this freshly accreted cold gas settles into a large disc-like system, not necessarily aligned to an older stellar component, that undergoes fragmentation and subsequent star formation, forming large clumps in the mass range 107-109 M. Galaxy formation is a complex process at this important epoch when most of the central baryons are being acquired through a range of different mechanisms - we highlight that a rapid mass loading epoch is required to fuel the fragmentation taking place in the massive arms in the outskirts of extended discs, an accretion mode that occurs naturally in the hierarchical assembly process at early epochs.

Original languageEnglish (US)
Pages (from-to)L64-L68
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume397
Issue number1
DOIs
StatePublished - Jul 2009
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: haloes

Fingerprint

Dive into the research topics of 'Disc formation and the origin of clumpy galaxies at high redshift'. Together they form a unique fingerprint.

Cite this