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What is the origin of the soft excess in active galactic nuclei?

Author
SOBOLEWSKA, Malgorzata A1 ; DONE, Chris1
[1] Department of Physics, University of Durham, South Road, Durham DHI 3LE, United Kingdom
Source

Monthly Notices of the Royal Astronomical Society. 2007, Vol 374, Num 1, pp 150-158, 9 p ; ref : 1/4 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
X-rays: galaxies accretion, accretion discs atomic processes galaxies: active galaxies: individual: 1H 0707-495 galaxies: individual: PG 1211+143
Keyword (fr)
Basse température Cosmologie Disque accrétion Déplacement vers le rouge Galaxies RX Galaxies Seyfert type 1 Galaxies actives Modèle Noyau galactique actif Noyau galaxies Processus atomique Quasar Rayon X mou Source RX cosmique Trou noir
Keyword (en)
Low temperature Cosmology Accretion disks Red shift X-ray galaxies Seyfert 1 galaxies Active galaxies Models Active galaxy nuclei Galaxy nuclei Atomic process Quasars Soft X radiation Cosmic x-ray sources Black holes
Keyword (es)
Baja temperatura Galaxias Seyfert tipo 1 Modelo Proceso atómico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18485758

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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