New multi-zoom method for N-body simulations : application to galaxy growth by accretion
- Author
- SEMELIN, B1 ; COMBES, F1
[1] Observatoire de Paris, LERMA, 61 Av. de l'Observatoire, 75014 Paris, France - Source
Astronomy and astrophysics (Berlin. Print). 2005, Vol 441, Num 1, pp 55-67, 13 p ; ref : 46 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: large-scale structure of Universe galaxies: evolution galaxies: formation galaxies: intergalactic medium galaxies: spiral
- Keyword (fr)
- Accrétion Cosmologie Effondrement Formation galaxies Galaxies spirales Gaz froid Gaz intergalactique Matière intergalactique Matière sombre Plan galactique Propriété géométrique Relation Tully Fisher Simulation numérique Structure grande échelle Système n corps Taux accrétion Evolution galaxies
- Keyword (en)
- Accretion Cosmology Collapse Galaxy formation Spiral galaxies Cold gas Intergalactic gas Intergalactic matter Dark matter Galactic planes Geometrical properties Tully Fisher relation Digital simulation Large-scale structure N body system Accretion rate Galaxy evolution
- Keyword (es)
- Desmoronamiento Gas frío Gas intergaláctico Propiedad geométrica Relación Tully Fisher Sistema n cuerpos Índice acreción Evolución galaxias
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17104142
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
10.1051/0004-6361:20042473 
https://dx.doi.org/10.1051/0004-6361:20042473
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