Warm-hot baryons comprise 5-10 per cent of filaments in the cosmic web.

Eckert, Dominique; Jauzac, Mathilde; Shan, HuanYuan; Kneib, Jean-Paul; Erben, Thomas; Israel, Holger; Jullo, Eric; Klein, Matthias; Massey, Richard; Richard, Johan; Tchernin, Céline

Eckert, Dominique; Jauzac, Mathilde; Shan, HuanYuan; Kneib, Jean-Paul; Erben, Thomas; Israel, Holger; Jullo, Eric; Klein, Matthias; Massey, Richard; Richard, Johan; Tchernin, Céline.

Afiliação

Eckert D; Department of Astronomy, University of Geneva, Chemin d'Ecogia 16, 1290 Versoix, Switzerland.
Jauzac M; INAF - IASF Milano, Via E. Bassini 15, 20133 Milan, Italy.
Shan H; Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK.
Kneib JP; Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu-Natal, Durban 4041, South Africa.
Erben T; Laboratoire d'Astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland.
Israel H; Laboratoire d'Astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland.
Jullo E; Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, 13388 Marseille, France.
Klein M; Argelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 Bonn, Germany.
Massey R; Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK.
Richard J; Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, 13388 Marseille, France.
Tchernin C; Argelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 Bonn, Germany.

Nature ; 528(7580): 105-7, 2015 Dec 03.

Article em En | MEDLINE | ID: mdl-26632589

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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nature Ano de publicação: 2015 Tipo de documento: Article País de afiliação: Suíça

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