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On the variation of black hole accretion disc radii as a function of state and accretion rate

Author
CABANAC, C1 ; FENDER, R. P1 ; DUNN, R. J. H1 2 ; KÖRDING, E. G1 3
[1] School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, United Kingdom
[2] Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
[3] AIM - Unité Mixte de Recherche CEA - CNRS - Université Paris VII - UMR 7158, CEA-Saclay, Service d'Astrophysique, 91191 Gif-sur-Yvette, France
Source

Monthly notices of the Royal Astronomical Society (Print). 2009, Vol 396, Num 3, pp 1415-1440, 26 p ; ref : 3/4 p

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Wiley-Blackwell, Malden, MA
Publication country
United States
Document type
Article
Language
English
Author keyword
X-rays: binaries accretion, accretion discs
Keyword (fr)
Accrétion Binaire RX Cosmologie Densité colonne Disque accrétion Incertitude Luminosité Modèle théorique Orbite circulaire Rayon X dur Rayon X mou Source RX binaire Source RX cosmique Taux accrétion Timing Trou noir
Keyword (en)
Accretion X-ray binary stars Cosmology Column density Accretion disks Uncertainty Luminosity Theoretical model Circular orbit Hard x radiation Soft X radiation Binary X ray source Cosmic x-ray sources Accretion rate Timing Black holes
Keyword (es)
Densidad columna Incertidumbre Modelo teórico Orbita circular Fuente RX binaria Índice acreción
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
21635078

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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