Thermal and chemical evolution of collapsing filaments

William J. Gray, Evan Scannapieco

Research output: Contribution to journalArticle

7 Citations (Scopus)

Abstract

Intergalactic filaments form the foundation of the cosmic web that connect galaxies together, and provide an important reservoir of gas for galaxy growth and accretion. Here we present very high resolution two-dimensional simulations of the thermal and chemical evolution of such filaments, making use of a 32 species chemistry network that tracks the evolution of key molecules formed from hydrogen, oxygen, and carbon. We study the evolution of filaments over a wide range of parameters including the initial density, initial temperature, strength of the dissociating UV background, and metallicity. In low-redshift, Z ≈ 0.1 Z filaments, the evolution is determined completely by the initial cooling time. If this is sufficiently short, the center of the filament always collapses to form a dense, cold core containing a substantial fraction of molecules. In high-redshift, Z = 10-3 Z filaments, the collapse proceeds much more slowly. This is mostly due to the lower initial temperatures, which lead to a much more modest increase in density before the atomic cooling limit is reached, making subsequent molecular cooling much less efficient. Finally, we study how the gravitational potential from a nearby dwarf galaxy affects the collapse of the filament and compare this to NGC 5253, a nearby starbursting dwarf galaxy thought to be fueled by the accretion of filament gas. In contrast to our fiducial case, a substantial density peak forms at the center of the potential. This peak evolves faster than the rest of the filament due to the increased rate at which chemical species form and cooling occurs. We find that we achieve similar accretion rates as NGC 5253 but our two-dimensional simulations do not recover the formation of the giant molecular clouds that are seen in radio observations.

Original languageEnglish (US)
Article number174
JournalAstrophysical Journal
Volume768
Issue number2
DOIs
StatePublished - May 10 2013

Fingerprint

chemical evolution
filaments
cooling
accretion
gas
dwarf galaxies
simulation
temperature
hydrogen
radio
oxygen
galaxies
chemical
carbon
radio observation
molecular clouds
gases
gravitational fields
metallicity
molecules

Keywords

  • galaxies: abundances
  • galaxies: dwarf
  • galaxies: evolution
  • galaxies: individual (NGC 5253)
  • galaxies: starburst
  • intergalactic medium

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Thermal and chemical evolution of collapsing filaments. / Gray, William J.; Scannapieco, Evan.

In: Astrophysical Journal, Vol. 768, No. 2, 174, 10.05.2013.

Research output: Contribution to journalArticle

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