36 research outputs found

    The forbidden high ionisation line region of the type 2 quasar Q1131+16: a clear view of the inner face of the torus?

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    We present spectroscopic observations of the type 2 quasar SDSS J11311.05+162739.5 (Q1131+16 hereafter; z=0.1732), which has the richest spectrum of forbidden high ionisation lines (FHIL, e.g. [Fe \textsc{vii}], [Fe \textsc{x}], [Fe \textsc{xi}] and [Ne \textsc{v}]) yet reported for an AGN, as well as unusually strong [O \textsc{iii}]λ\lambda4363 emission. The study of this object provides a rare opportunity to investigate the physical conditions and kinematics of the region(s) emitting the FHILs. By comparison with photoionisation model results, we find that the FHIL region has high densities (105.5^{5.5} << nHn_H <108.0<10^{8.0} cm\textsuperscript{-3}) and ionisation parameters (-1.5 << log[U] << 0), yet its kinematics are similar to those of the low ionisation emission line region detected in the same object (FWHM \sim 360±\pm30 km/s), with no evidence for a significant shift between the velocity centroid of the FHILs and the rest frame of the host galaxy. The deduced physical conditions lie between those of the Broad-Line (nH_H>109>10^9 cm\textsuperscript{-3}) and Narrow-Line Regions (nHn_H<106<10^6 cm\textsuperscript{-3}) of active galactic nuclei (AGN), and we demonstrate that the FHIL regions must be situated relatively close to the illuminating AGN (0.32 << rFHILr_{FHIL} << 50pc). We suggest that the inner torus wall is the most likely location for the FHIL region, and that the unusual strength of the FHILs in this object is due to a specific viewing angle of the far wall of the torus, coupled with a lack of dust on larger scales that might otherwise obscure our view of the torus.Comment: Accepted for publication in the Monthly Notices of the Royal Astronomical Society (3rd of March 2011). 23 Pages (including tables 5 and 6 in the source file), 21 figure

    A Model for Type 2 Coronal Line Forest (CLiF) AGNs

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    We present a model for the classification of Coronal Line Forest Active Galactic Nuclei (CLiF AGNs). CLiF AGNs are of special interest due to their remarkably large number of emission lines, especially forbidden highionization lines (FHILs). Rose et al. suggest that their emission is dominated by reflection from the inner wall of the obscuring region rather than direct emission from the accretion disk. This makes CLiF AGNs laboratories to test AGN-torus models. Modeling an AGN as an accreting supermassive black hole surrounded by a cylinder of dust and gas, we show a relationship between the viewing angle and the revealed area of the inner wall. From the revealed area, we can determine the amount of FHIL emission at various angles. We calculate the strength of [Fe VII]λ6087 emission for a number of intermediate angles (30°, 40°, and 50°) and compare the results with the luminosity of the observed emission line from six known CLiF AGNs. We find that there is good agreement between our model and the observational results. The model also enables us to determine the relationship between the type 2:type 1 AGN fraction vs the ratio of torus height to radius, h/r

    Descemet membrane endothelial keratoplasty

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    Expert opinion in the management of aqueous Deficient Dry Eye Disease (DED) Cornea and external eye diseases

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    © 2015 Sy et al.Background: Dry eye disease (DED) affects millions of people worldwide. There are a variety of new treatments beyond traditional therapies such as preservative free artificial tears. Here, we conduct a survey to identify the most common tr

    Training clinicians treating HIV to diagnose cytomegalovirus retinitis

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    © 2014, World Health Organization, All rights reserved.Problem Acquired immunodeficiency syndrome (AIDS)-related cytomegalovirus (CMV) retinitis continues to be a neglected source of blindness in resource-poor settings. The main issue is lack of capacity
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