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The thermal history of the intergalactic medium

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Schaye, Joop, Theuns, Tom, Rauch, Michael, Efstathiou, George, Sargent, Wallace L.W.·2000·Monthly Notices of the Royal Astronomical Society

Abstract

At redshifts z ≳ 2, most of the baryons reside in the smooth intergalactic medium which is responsible for the low column density Lyα forest. This photoheated gas follows a tight temperature-density relation which introduces a cut-off in the distribution of widths of the Lyα absorption lines (b-parameters) as a function of column density. We have measured this cut-off in a sample of nine high-resolution, high signal-to-noise ratio quasar spectra and determined the thermal evolution of the intergalactic medium in the redshift range 2.0–4.5. At a redshift z∼3, the temperature at the mean density shows a peak and the gas becomes nearly isothermal. We interpret this as evidence for the reionization of He ii.

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Metadata

Authors
Schaye, J., Theuns, T., Rauch, M., Efstathiou, G., & Sargent, W. L. W.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2000-11
Volume
318
Issue
3
Pages
817-826
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2029248679
Cited by
395
References
0
FWCI
15.07
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The thermal history of the intergalactic medium. https://app.cochat.ai/papers/10.1046/j.1365-8711.2000.03815.x
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Schaye, J., Theuns, T., Rauch, M., Efstathiou, G., & Sargent, W. L. W. (2000). The thermal history of the intergalactic medium. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2000.03815.x

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