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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DOI
10.1086/430699 
https://dx.doi.org/10.1086/430699
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