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A systematic look at the very high and low/hard state of GX 339-4 : constraining the black hole spin with a new reflection model

Author
REIS, R. C1 ; FABIAN, A. C1 ; ROSS, R. R2 ; MINIUTTI, G1 3 ; MILLER, J. M4 ; REYNOLDS, C5
[1] Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, United Kingdom
[2] Physics Department, College of the Holy Cross, Worcester, MA 01610, United States
[3] Laboratoire Astroparticule et Cosmologie (APC), UMR 7164, 10 Rue A. Domon et L. Duquet, 75205 Paris, France
[4] Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, United States
[5] Department of Astronomy, The University of Maryland, College Park, MD 20742, United States
Source

Monthly Notices of the Royal Astronomical Society. 2008, Vol 387, Num 4, pp 1489-1498, 10 p ; ref : 1/2 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: individual: GX 339-4 accretion, accretion disc black hole physics
Keyword (fr)
Continuum Cosmologie Disque accrétion Modèle Observation simultanée Orbite circulaire Rayonnement corps noir Rotation rapide Spectre RX Trou noir
Keyword (en)
Continuum Cosmology Accretion disks Models Simultaneous observation Circular orbit Blackbody radiation Rapid rotation X-ray spectra Black holes
Keyword (es)
Continuo Modelo Observación simultánea Orbita circular Rotación rápida
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20488575

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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