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Simulations of thermally broadened H i Ly α absorption arising in the warm-hot intergalactic medium

Author
RICHTER, P1 ; FANG, T2 ; BRYAN, G. L3
[1] Argelander-Institut für Astronomic, Universität Bonn, Aufdem Hügel 71, 53121 Bonn, Germany
[2] Department of Astronomy, University of California at Berkeley, 601 Campbell Hall, Berkeley, CA 94720, United States
[3] Department of Physics, University of Oxford, Keble Road, Oxford OX13RH, United Kingdom
Source

Astronomy and astrophysics (Berlin. Print). 2006, Vol 451, Num 3, pp 767-776, 10 p ; ref : 21 ref

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
cosmology: miscellaneous large-scale structure of Universe methods: numerical
Keyword (fr)
Absorption UV Baryon Composé trace Cosmologie Densité colonne Déplacement vers le rouge Elargissement raie Gaz ionisé Largeur raie Matière intergalactique Modèle hydrodynamique Méthode numérique Quasar Raie absorption Simulation numérique Structure grande échelle Turbulence
Keyword (en)
Ultraviolet absorption Baryons Trace compound Cosmology Column density Red shift Line broadening Ionized gases Line widths Intergalactic matter Hydrodynamic model Numerical method Quasars Absorption line Digital simulation Large-scale structure Turbulence
Keyword (es)
Absorción UV Compuesto huella Densidad columna Método numérico Raya absorción
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17773102

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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