English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/170193
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:


The XMM-Newton Bright Survey sample of absorbed quasars: X-ray and accretion properties

AuthorsBallo, Lucía ; Severgnini, P.; Della Ceca, R.; Caccianiga, A.; Vignali, C.; Carrera, Francisco J. ; Corral, Amalia ; Mateos, Silvia
KeywordsInfrared: galaxies
Galaxies: active
Quasars: general
X-rays: galaxies
Issue Date2014
PublisherRoyal Astronomical Society
Oxford University Press
CitationMonthly Notices of the Royal Astronomical Society 444(3): 2580-2598 (2014)
AbstractAlthough absorbed quasars are extremely important for our understanding of the energetics of the Universe, the main physical parameters of their central engines are still poorly known. In this work, we present and study a complete sample of 14 quasars (QSOs) that are absorbed in the X-rays (column density NH > 4 × 1021 cm−2 and X-ray luminosity L 2-10 keV > 1044 ergs−1; XQSO2) belonging to the XMM–Newton Bright Serendipitous Survey (XBS). From the analysis of their ultraviolet-to-mid-infrared spectral energy distribution, we can separate the nuclear emission from the host galaxy contribution, obtaining a measurement of the fundamental nuclear parameters, like the mass of the central supermassive black hole and the value of Eddington ratio, λ Edd. Comparing the properties of XQSO2s with those previously obtained for the X-ray unabsorbed QSOs in the XBS, we do not find any evidence that the two samples are drawn from different populations. In particular, the two samples span the same range in Eddington ratios, up to λ Edd ∼ 0.5; this implies that our XQSO2s populate the ‘forbidden region’ in the so-called ‘effective Eddington limit paradigm’. A combination of low grain abundance, presence of stars inwards of the absorber, and/or anisotropy of the disc emission can explain this result.
Publisher version (URL)https://doi.org/10.1093/mnras/stu1628
Identifiersdoi: 10.1093/mnras/stu1628
e-issn: 1365-2966
issn: 0035-8711
Appears in Collections:(IFCA) Artículos
Files in This Item:
File Description SizeFormat 
XMM-Newproper.pdf1,33 MBAdobe PDFThumbnail
Show full item record
Review this work

Related articles:

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.