Radial-orbit instability of a family of anisotropic Hernquist models with and without a supermassive black hole
- Author
- BUYLE, P1 ; VAN HESE, E1 ; DE RIJCKE, S1 ; DEJONGHE, H1
[1] Slerrenkundig Observatorium, Ghent University, Krijgslaan 281, S9, 9000 Ghent, Belgium - Source
Monthly Notices of the Royal Astronomical Society. 2007, Vol 375, Num 4, pp 1157-1170, 14 p ; ref : 1/4 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- galaxies: kinematics and dynamics methods: N-body simulations stellar dynamics
- Keyword (fr)
- Algorithme Anisotropie Cinématique Cosmologie Dynamique stellaire Galaxies Instabilité Modèle dynamique Modèle sphérique Orbite Particule sphérique Simulation numérique Système n corps Trou noir supermassif Trou noir
- Keyword (en)
- Algorithms Anisotropy Kinematics Cosmology Stellar dynamics Galaxies Instability Dynamic model Spherical model Orbits Spherical particle Digital simulation N body system Supermassive black hole Black holes
- Keyword (es)
- Modelo dinámico Partícula esférica Sistema n cuerpos Agujero negro supermasivo
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18563465
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
10.1111/j.1365-2966.2006.11396.x 
https://dx.doi.org/10.1111/j.1365-2966.2006.11396.x
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