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A soft X-ray study of type I active galactic nuclei observed with Chandra high-energy transmission grating spectrometer

Author
MCKEMAN, B1 2 ; YAQOOB, T3 4 ; REYNOLDS, C. S5
[1] Department of Science, Borough of Manhattan Community College, City University of New York, New York, NY 10007, United States
[2] Hayden Associate, Hayden Planetarium, Department of Astrophysics, American Museum of Natural History, New York, NY 10024, United States
[3] Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, United States
[4] Laboratory for High Energy Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, United States
[5] Department of Astronomy, University of Maryland, College Park, MD 20742, United States
Source

Monthly Notices of the Royal Astronomical Society. 2007, Vol 379, Num 4, pp 1359-1372, 14 p ; ref : 3/4 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
Galaxy: disc X-rays: galaxies galaxies: Seyfert galaxies: active techniques: spectroscopic
Keyword (fr)
Borne supérieure Cinématique Cosmologie Densité colonne Facteur remplissage Galaxies RX Galaxies Seyfert Galaxies actives Galaxies disques Ionisation multiple Noyau galactique actif Noyau galaxies Rayon X mou Source RX cosmique Spectre RX Taux accrétion Trou noir supermassif
Keyword (en)
Upper bound Kinematics Cosmology Column density Fill factor X-ray galaxies Seyfert galaxies Active galaxies Disk galaxies Multiple ionization Active galaxy nuclei Galaxy nuclei Soft X radiation Cosmic x-ray sources X-ray spectra Accretion rate Supermassive black hole
Keyword (es)
Cota superior Densidad columna Ionización múltiple 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
18977227

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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