Effect of metallicity on X-ray emission from the warm-hot intergalactic medium

E. Ursino, Massimiliano Galeazzi, M. Roncarelli

Research output: Contribution to journalArticle

11 Citations (Scopus)

Abstract

Hydrodynamic simulations predict that a significant fraction of the gas in the current universe is in the form of high temperature, highly ionized plasma emitting and absorbing primarily in the soft X-ray and UV bands, dubbed the warm-hot intergalactic medium (WHIM). Its signature should be observable in redshifted emission and absorption lines from highly ionized elements. To determine the expected WHIM emission in the soft X-ray band we used the output of a large scale smoothed particle hydrodynamic simulation to generate images and spectra with angular resolution of 14″ and energy resolution of 1 eV. The current biggest limit of any hydrodynamic simulation in predicting the X-ray emission comes from metal diffusion. In our investigation, by using four different models for the WHIM metallicity we have found a strong dependence of the emission on the model used, with differences up to almost an order of magnitude. For each model, we have investigated the redshift distribution and angular scale of the emission, confirming that most photons come from redshift z <1.2 and that the emission has a typical angular scale of less than a few arcminutes. We also compared our simulations with the few currently available observations and found that, within the variation of the metallicity models, our predictions are in good agreement with current constraints on the WHIM emission, and at this time the weak experimental constraints on the WHIM emission are not sufficient to exclude any of the models used.

Original languageEnglish (US)
Pages (from-to)46-58
Number of pages13
JournalAstrophysical Journal
Volume721
Issue number1
DOIs
StatePublished - Sep 20 2010

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intergalactic media
metallicity
x rays
hydrodynamics
simulation
effect
angular resolution
universe
signatures
plasma
output
metal
photons
prediction
predictions
gases
gas
metals

Keywords

  • Diffuse radiation
  • Intergalactic medium
  • Large-scale structure of universe
  • Methods: numerical
  • Radiation mechanisms: thermal
  • X-rays: diffuse background

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics
  • Nuclear and High Energy Physics

Cite this

Effect of metallicity on X-ray emission from the warm-hot intergalactic medium. / Ursino, E.; Galeazzi, Massimiliano; Roncarelli, M.

In: Astrophysical Journal, Vol. 721, No. 1, 20.09.2010, p. 46-58.

Research output: Contribution to journalArticle

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