Turbulent gas motions in galaxy cluster simulations : the role of smoothed particle hydrodynamics viscosity
- Author
- DOLAG, K1 2 ; VAZZA, F1 ; BRUNETTI, G3 ; TORMEN, G1
[1] Dipartimento di Astronomia, Universita di Padova, vicolo dell'Osservatorio 2, 35122 Padova, Italy
[2] Max-Planck-Institut für Astrophysik, Garching, Germany
[3] INAF, Istituto di Radioastronomia, via P.Gobetti 101, 40129 Bologna, Italy - Source
Monthly Notices of the Royal Astronomical Society. 2005, Vol 364, Num 3, pp 753-772, 20 p ; ref : 49 ref
- 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: clusters: general hydrodynamics methods: numerical turbulence
- Keyword (fr)
- Accélération particule Amas galaxies Aplatissement Champ vitesse Densité énergie Emission radioélectrique Energie cinétique Entropie Instabilité Luminosité Matière intraamas Modèle particule Mouvement aléatoire Méthode SPH Méthode numérique Onde MHD Onde choc Turbulence Viscosité
- Keyword (en)
- Particle acceleration Galaxy clusters Flattening Velocity fields Energy density Radio emission Kinetic energy Entropy Instability Luminosity Intracluster matter Particle models Random motion Smoothed particle hydrodynamics method Numerical method MHD waves Shock waves Turbulence Viscosity
- Keyword (es)
- Aceleración partícula Aplanamiento Emisión radioeléctrica Materia intracúmulo Movimiento aleatorio Método SPH Método numérico
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17326552
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.1365-2966.2005.09630.x 
https://dx.doi.org/10.1111/j.1365-2966.2005.09630.x
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