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Compressible turbulence in galaxy clusters: physics and stochastic particle re-acceleration

Author
BRUNETTI, G1 ; LAZARIAN, A2
[1] INAF - Istituto di Radioastronomia, via Gobetti 101, 40129 Bologna, Italy
[2] Department of Astronomy, University of Wisconsin at Madison, 5534 Sterling Hall, 475 North Charter Street, Madison, WI 53706, United States
Source

Monthly Notices of the Royal Astronomical Society. 2007, Vol 378, Num 1, pp 245-275, 31 p ; ref : 1 p.3/4

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
X-rays: general acceleration of particles galaxies: clusters: general radiation mechanisms: non-thermal radio continuum: general turbulence
Keyword (fr)
Accélération particule Amas galaxies Amortissement Champ magnétique Continuum Couplage résonnant Célérité son Diffusion(transport) Electron relativiste Galaxies en coalescence Ligne force Matière intraamas Modèle Particule relativiste Plasma turbulent Rayonnement non thermique Transfert énergie Turbulence isotrope Viscosité
Keyword (en)
Particle acceleration Galaxy clusters Damping Magnetic fields Continuum Resonant coupling Sound velocity Diffusion Relativistic electron Merging galaxies Field line Intracluster matter Models Relativistic particle Turbulent plasma Nonthermal radiation Energy transfer Isotropic turbulence Viscosity
Keyword (es)
Aceleración partícula Continuo Acoplamiento resonante Electrón relativista Galaxias en coalescencia Línea fuerza Materia intracúmulo Modelo Partícula relativista Plasma turbulento Turbulencia isótropa
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18800149

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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