High-metallicity, photoionized gas in intergalactic large-scale filaments

Bastien Aracil, Todd M. Tripp, David V. Bowen, Jason X. Prochaska, Hsiao Wen Chen, Brenda L. Frye

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37 Scopus citations

Abstract

ABSTRACT We present high-resolution ultraviolet spectra of absorption-line systems towards the low-z quasi-stellar object (QSO) HS 0624+6907 (z QSO= 0.3700). Coupled with ground-based imaging and spectroscopic galaxy redshifts, we find evidence that many of these absorbers do not arise in galaxy haloes but rather are truly intergalactic gas clouds distributed within large-scale structures, and moreover, the gas is cool (T < 105 K) and has relatively high metallicity (Z > 0.9 Z ). Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) data reveal a dramatic cluster of 13 H i Lyman α (Lyα) lines within a 1000 km s-1 interval at z abs= 0.0635. We find 10 galaxies at this redshift with impact parameters ranging from ρ= 135 h-170 kpc to 1.37 h-170 Mpc. The velocities and velocity spread of the Lyα lines in this complex are unlikely to arise in the individual haloes of the nearby galaxies; instead, we attribute the absorption to intragroup medium gas, possibly from a large-scale filament viewed along its long axis. Contrary to theoretical expectations, this gas is not the shock-heated warm-hot intergalactic medium (WHIM); the width of the Lyα lines all indicate a gas temperature T≪ 105 K, and metal lines detected in the Lyα complex also favour photoionized, cool gas. No O vi absorption lines are evident, which is consistent with photoionization models. Remarkably, the metallicity is near-solar, [M/H]=-0.05 ± 0.4 (2σ uncertainty), yet the nearest galaxy which might pollute the intergalactic medium is at least 135 h-170 kpc away. Tidal stripping from nearby galaxies appears to be the most likely origin of this highly enriched, cool gas. More than six Abell galaxy clusters are found within 4°of the sight line suggesting that the QSO line of sight passes near a node in the cosmic web. At z≈ 0.077, we find absorption systems as well as galaxies at the redshift of the nearby clusters Abell 564 and Abell 559. We conclude that the sight line pierces a filament of gas and galaxies feeding into these clusters. The absorber at zabs= 0.075 73 associated with Abell 564/559 also has a high metallicity with [C/H] > -0.6, but again the closest galaxy is relatively far from the sight line (ρ= 293 h-170 kpc). The Doppler parameters and H i column densities of the Lyα lines observed along the entire sight line are consistent with those measured towards other low-z QSOs, including a number of broad (b > 40 km s-1) Lyα lines.

Original languageEnglish (US)
Pages (from-to)139-155
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume367
Issue number1
DOIs
StatePublished - Mar 2006
Externally publishedYes

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Keywords

  • Galaxies: abundances
  • Intergalactic medium
  • Large-scale structure of Universe

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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