A synchrotron self-Compton scenario for the very high energy γ-ray emission of the radiogalaxy M 87 Unifying the TeV emission of blazars and other AGNs?
- Author
- LENAIN, J.-P1 ; BOISSON, C1 ; SOL, H1 ; KATARZYNSKI, K2
[1] LUTH, Observatoire de Paris, CNRS, Université Paris Diderot; 5 Place Jules Janssen, 92190 Meudon, France
[2] Toruń Centre for Astronomy, Nicolaus Copernicus University, ul. Gagarina 11, 87100 Toruri, Poland - Source
Astronomy and astrophysics (Berlin. Print). 2008, Vol 478, Num 1, pp 111-120, 10 p ; ref : 1/2 p
- 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
- galaxies: active galaxies: individual: M 87 gamma rays: theory radiation mechanisms: non-thermal
- Keyword (fr)
- Angle observation Blazar Cosmologie Domaine énergie TeV Emission gamma Galaxies actives Jet Magnétohydrodynamique relativiste Modèle MHD Modèle standard Noyau galactique actif Noyau galaxies Performance Plasma Quasar Radiogalaxies Radiosource cosmique Rayonnement gamma Rayonnement non thermique Source extragalactique Source étendue Spectre gamma Trou noir supermassif Trou noir Très haute énergie Variabilité
- Keyword (en)
- Viewing angle Blazar Cosmology TeV range Gamma emission Active galaxies Jets Relativistic magnetohydrodynamics MHD model Standard model Active galaxy nuclei Galaxy nuclei Performance Plasma Quasars Radio galaxies Cosmic radio sources Gamma radiation Nonthermal radiation Extragalactic source Extended source Gamma spectra Supermassive black hole Black holes Very high energy Variability
- Keyword (es)
- Angulo observación Emisión gamma Magnetohidrodinámica relativista Modelo MHD Fuente extragaláctica Fuente alargada Agujero negro supermasivo Energía muy alta Variabilidad
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19985347
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
10.1051/0004-6361:20077995 
https://dx.doi.org/10.1051/0004-6361:20077995
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