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Re-condensation from an ADAF into an inner disk : the intermediate state of black hole accretion?

Author
MEYER, F1 ; LIU, B. F2 ; MEYER-HOFMEISTER, E1
[1] Max-Planck-Institut für Astrophysik, Karl-Schwarzschildstr. 1, 85740 Garching, Germany
[2] National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming 650011, China
Source

Astronomy and astrophysics (Berlin. Print). 2007, Vol 463, Num 1, pp 1-9, 9 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: binaries accretion, accretion disks black hole physics stars: individual: Cyg X-1
Keyword (fr)
Accrétion Advection Binaire RX Condensation Conduction thermique Cosmologie Disque accrétion Etat transition Evaporation Luminosité Modèle Source RX binaire Source RX cosmique Source RX transitoire Taux accrétion Trou noir supermassif Trou noir
Keyword (en)
Accretion Advection X-ray binary stars Vapor condensation Thermal conduction Cosmology Accretion disks Transition state Evaporation Luminosity Models Binary X ray source Cosmic x-ray sources Transient X ray source Accretion rate Supermassive black hole Black holes
Keyword (es)
Estado transitorio Modelo Fuente RX binaria Fuente RX transitoria Índice acreción Agujero negro supermasivo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18485127

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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