Author
Listed:
- Dominique Eckert
(University of Geneva, Chemin d’Ecogia 16
INAF – IASF Milano, Via E. Bassini 15)
- Mathilde Jauzac
(Institute for Computational Cosmology, Durham University
Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu-Natal)
- HuanYuan Shan
(Laboratoire d’Astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny)
- Jean-Paul Kneib
(Laboratoire d’Astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny
Aix Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326)
- Thomas Erben
(Argelander-Institut für Astronomie, Auf dem Hügel 71)
- Holger Israel
(Institute for Computational Cosmology, Durham University)
- Eric Jullo
(Aix Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326)
- Matthias Klein
(Argelander-Institut für Astronomie, Auf dem Hügel 71)
- Richard Massey
(Institute for Computational Cosmology, Durham University)
- Johan Richard
(CRAL, Observatoire de Lyon, Université Lyon 1)
- Céline Tchernin
(University of Geneva, Chemin d’Ecogia 16)
Abstract
In the local Universe, the census of all observed baryons falls short of the estimated number by a factor of two, and simulations have indicated that the missing baryons reside throughout the filaments of the cosmic web; X-ray observations of filamentary structures associated with the galaxy cluster Abell 2744 now find that 5 to 10 per cent of the filament mass is in the form of baryonic gas.
Suggested Citation
Dominique Eckert & Mathilde Jauzac & HuanYuan Shan & Jean-Paul Kneib & Thomas Erben & Holger Israel & Eric Jullo & Matthias Klein & Richard Massey & Johan Richard & Céline Tchernin, 2015.
"Warm–hot baryons comprise 5–10 per cent of filaments in the cosmic web,"
Nature, Nature, vol. 528(7580), pages 105-107, December.
Handle:
RePEc:nat:nature:v:528:y:2015:i:7580:d:10.1038_nature16058
DOI: 10.1038/nature16058
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