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THE EXISTENCE OF INNER COOL DISKS IN THE LOW/HARD STATE OF ACCRETING BLACK HOLES

Author
LIU, B. F1 ; TAAM, Ronald E2 3 4 ; MEYER-HOFMEISTER, E5 ; MEYER, F5
[1] National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming, 650011 Yunnan, China
[2] Department of Physics and Astronomy, Northwestern University, Evanston, IL 60208, United States
[3] Institute of Astronomy and Astrophysics, Academia Sinica, Academia Sinica and National Tsing Hua University, Hsinchu 30013, Taiwan, Province of China
[4] Theoretical Institute for Advanced Research in Astrophysics, Academia Sinica and National Tsing Hua University, Hsinchu 30013, Taiwan, Province of China
[5] Max-Planck-Institut für Astrophysik, 85740 Garching, Germany
Source

The Astrophysical journal. 2007, Vol 671, Num 1, pp 695-705, 11 p ; 1 ; ref : 1/2 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
X-rays: binaries X-rays: stars accretion, accretion disks black hole physics stars: individual (GX 339-4, SWIFT J1753.5-0127)
Keyword (fr)
Binaire RX Cosmologie Disque accrétion Source RX binaire Source RX cosmique Trou noir
Keyword (en)
X-ray binary stars Cosmology Accretion disks Binary X ray source Cosmic x-ray sources Black holes
Keyword (es)
Fuente RX binaria
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19924483

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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