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A possible interpretation of the Seyfert-like component in 3C 273 X-ray spectrum

Author
PIETRINI, P1 ; TORRICELLI-CIAMPONI, G2
[1] Dipartimento di Astronomia e Scienza dello Spazio, Largo E. Fermi 2, 50125 Firenze, Italy
[2] INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
Source

Astronomy and astrophysics (Berlin. Print). 2008, Vol 479, Num 2, pp 365-376, 12 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
X-rays: galaxies galaxies: active galaxies: nuclei quasars: individual: 3C 273 radiation mechanisms: non-thermal
Keyword (fr)
Corrélation Emission RX Galaxies RX Galaxies actives Jet Loi puissance Modèle Mécanisme rayonnement Noyau galactique actif Noyau galaxies Quasar Raie émission Source RX cosmique Spectre RX
Keyword (en)
Correlations X ray emission X-ray galaxies Active galaxies Jets Power law Models Radiation mechanism Active galaxy nuclei Galaxy nuclei Quasars Emission line Cosmic x-ray sources X-ray spectra
Keyword (es)
Emisión RX Ley poder Modelo Mecanismo radiación Raya emisión
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20066006

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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