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Massive galaxies and extremely red objects at z = 1-3 in cosmological hydrodynamic simulations : Near-infrared properties

Author
NAGAMINE, Kentaro1 ; RENYUE CEN2 ; HERNQUIST, Lars3 ; OSTRIKER, Jeremiah P2 ; SPRINGEL, Volker4
[1] University of California, San Diego, Center for Astrophysics and Space Sciences, 9500 Gilman Drive, La Jolla, CA 92093-0424, United States
[2] Princeton University Observatory, Princeton, NJ 08544, United States
[3] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, United States
[4] Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85740 Garching bei Munchen, Germany
Source

The Astrophysical journal. 2005, Vol 627, Num 2, pp 608-620, 13 p ; 1 ; ref : 122 ref

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
cosmology: theory galaxies: evolution galaxies: formation methods: numerical stars: formation
Keyword (fr)
Cosmologie Formation galaxies Formation stellaire Galaxies Modèle hydrodynamique Méthode numérique Simulation numérique Evolution galaxies
Keyword (en)
Cosmology Galaxy formation Star formation Galaxies Hydrodynamic model Numerical method Digital simulation Galaxy evolution
Keyword (es)
Método numérico Evolución galaxias
Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17047012

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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