Radio signature of cosmological structure formation shocks
- Author
- HOEFT, Matthias1 ; BRIIGGEN, Marcus1
[1] International University Bremen, Campus Ring 1, 28759 Bremen, Germany - Source
Monthly Notices of the Royal Astronomical Society. 2007, Vol 375, Num 1, pp 77-91, 15 p ; ref : 1 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
- diffuse radiation galaxies: clusters: general methods: analytical radiation mechanisms: non-thermal radio continuum: general
- Keyword (fr)
- Accrétion Amas galaxies Borne supérieure Champ magnétique Continuum Electron relativiste Emission radioélectrique Halo radio Matière intraamas Méthode analytique Observable Onde choc Rayonnement non thermique Rayonnement synchrotron Reste supernova
- Keyword (en)
- Accretion Galaxy clusters Upper bound Magnetic fields Continuum Relativistic electron Radio emission Radio halo Intracluster matter Analytical method Observables Shock waves Nonthermal radiation Synchrotron radiation Supernova remnants
- Keyword (es)
- Cota superior Continuo Electrón relativista Emisión radioeléctrica Halo radio Materia intracúmulo Método analítico
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18519093
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.1365-2966.2006.11111.x 
https://dx.doi.org/10.1111/j.1365-2966.2006.11111.x
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