IMPROVED REFLECTION MODELS OF BLACK HOLE ACCRETION DISKS: TREATING THE ANGULAR DISTRIBUTION OF X-RAYS

Record Type
Journal Articles
Full Title
IMPROVED REFLECTION MODELS OF BLACK HOLE ACCRETION DISKS: TREATING THE ANGULAR DISTRIBUTION OF X-RAYS
Author(s)
Garcia J, Dauser T, Lohfink A, Kallman T, Steiner J, McClintock J, Brenneman L, Wilms J, Eikmann W, Reynolds C, Tombesi F
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2014 Feb 20
DOI
10.1088/0004-637X/782/2/76
ISSN
0004-637X
Volume
782
Issue
2
Page Count
14
Article Number
76
Keyword(s)
Astronomy & Astrophysics, accretion, accretion disks, black hole physics, galaxies: individual (Ark 120), line: formation, radiative transfer, X-rays: general, ACTIVE GALACTIC NUCLEI, K-ALPHA LINE, FLUORESCENT IRON LINES, XMM-NEWTON, COLD MATTER, SPECTRAL VARIABILITY, COMPTON REFLECTION, SEYFERT-GALAXIES, LOW/HARD STATE, STRONG GRAVITY
Citation
Garcia J, Dauser T, Lohfink A, Kallman T, Steiner J, McClintock J, Brenneman L, Wilms J, Eikmann W, Reynolds C, et al. IMPROVED REFLECTION MODELS OF BLACK HOLE ACCRETION DISKS: TREATING THE ANGULAR DISTRIBUTION OF X-RAYS. ASTROPHYS J. 2014;782 (2):14.
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