Durham University

About: Durham University is a education organization based out in Durham, United Kingdom. It is known for research contribution in the topics: Population & Galaxy. The organization has 39385 authors who have published 82311 publications receiving 3110994 citations. The organization is also known as: University of Durham & Gallery of Durham University.

Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population

Abstract: In this chapter we aim to address the question: how common are kilo-parsec scale ionised outflows in the host galaxies of powerful active galactic nuclei (AGN; i.e., quasars) and what are their properties (e.g., spatial extents, morphologies and energetics)? We select 16 targets for spatially-resolved spectroscopy (i.e., integral field unit [IFU] observations) from a well-constrained parent sample of \(\approx \)24,000 AGN. This means that we can place our observations into the context of the overall AGN population and therefore learn about the population as a whole. Our targets are \(z<0.2\) type 2 quasars that are radio-quiet, with star formation rates (\(\lesssim \)[10–100]\(\mathrm{M}_{\odot }\,\mathrm{yr}^{-1}\)) that are consistent with normal star-forming galaxies. We present Gemini-GMOS IFU observations covering the [O iii]\(\lambda \lambda 4959,5007\) and H\(\beta \) emission lines. We find high-velocity ionised gas (velocity widths \({\approx }600\)–1500 km s\(^{-1}\); maximum velocities \({\le }1700\) km s\(^{-1}\)) with observed spatial extents of \(\gtrsim \)(6–16) kpc in all targets. We show that our targets are representative of \(z<0.2\), type 2 quasars and that ionised outflows are not only common but also in \(\ge \)70 % (3\(\sigma \) confidence) of cases, they are extended over kiloparsec scales. Both star formation and AGN activity appear to be energetically viable to drive the outflows and we find no definitive evidence that favours one process over the other. Although uncertain, we derive mass outflow rates (typically \({\approx }10 \times \) the SFRs), kinetic energies (\({\approx }0.5\)–10 % of \(L_{\mathrm{AGN}}\)) and momentum rates (typically \({\gtrsim }[10\)–\(20]\times L_{\mathrm{AGN}}/c\)) consistent with theoretical models that predict that AGN-driven outflows play a significant role in shaping the evolution of galaxies.

The X-Ray Spectral Properties of SCUBA Galaxies

Abstract: Deep SCUBA surveys have uncovered a large population of massive submillimeter-emitting galaxies (SMGs; f850μm 4 mJy) at z 1. Although it is generally believed that these galaxies host intense star formation activity, there is growing evidence that a substantial fraction also harbor an active galactic nucleus (AGN; i.e., an accreting super-massive black hole [SMBH]). We present here possibly the strongest evidence for this viewpoint to date: the combination of ultradeep X-ray observations (the 2 Ms Chandra Deep Field-North) and deep Keck spectroscopic data of SMGs with radio counterparts. We find that the majority (≈75%) of these radio-selected spectroscopically identified SMGs host AGN activity; the other ≈25% have X-ray properties consistent with star formation (X-ray-derived star formation rates of ≈1300-2700 M☉ yr-1). The AGNs have properties generally consistent with those of nearby luminous AGNs (Γ ≈ 1.8 ± 0.5, NH ≈ 1020-1024 cm-2, and LX ≈ 1043-1044.5 ergs s-1), and the majority (≈80%) are heavily obscured (NH 1023 cm-2). We construct composite rest-frame 2-20 keV spectra for three different obscuration classes [NH 5 × 1023 cm-2], which reveal features not seen in the individual X-ray spectra. An ≈1 keV equivalent width Fe Kα emission line is seen in the composite X-ray spectrum of the most heavily obscured AGNs, suggesting Compton-thick or near Compton-thick absorption. Even taking into account the effects of absorption, we find that the average X-ray to far-IR luminosity ratio of the AGN-classified SMGs (LX/LFIR = 0.004) is approximately 1 order of magnitude below that found for typical quasars. This result suggests that intense star formation activity (of order ≈1000 M☉ yr-1) dominates the bolometric output of these SMGs. However, we also explore the possibility that the X-ray to far-IR luminosity ratio of the AGN components is intrinsically less than that found for typical quasars and postulate that some SMGs may be AGN dominated. We investigate the implications of our results for the growth of massive black holes, discuss the prospects for deeper X-ray observations, and explore the scientific potential offered by the next generation of X-ray observatories.

Intertrochanteric femoral fractures. Mechanical failure after internal fixation

Abstract: In a prospective study we assessed the causes of mechanical failure in a series of 230 intertrochanteric femoral fractures which had been internally fixed with either a sliding hip screw or a Kuntscher Y-nail. The overall rate of mechanical failure was 16.5%; cutting-out of the implant from the femoral head was the cause in three-quarters of the instances. Implants placed posteriorly in the femoral head cut out more often (27%) than those placed centrally (7%). The cut-out rate was also determined by the quality of the fracture reduction, but age, walking ability and bone density (assessed by the Singh grade and metacarpal indices) had no significant influence. We conclude that these fractures should be reduced as accurately as possible and it is imperative that the implant is placed centrally within the femoral head.

Disgusted subjects: the making of middle‐class identities

Abstract: Although the classed dimensions of ‘taste’ have, following Bourdieu, been widely discussed, expressions of disgust at perceived violations of taste have been less frequently considered in relation to class. This paper considers various expressions of disgust at white working-class existence and explores what they might tell us about middle-class identities and identifications. I argue that the narratives of decline and of lack present in such representations can be seen in terms of a long-standing middle-class project of distinguishing itself. Drawing on Bourdieu's critique of Kantian aesthetics, I argue that the ownership of ‘taste’ is understood as reflecting true humanity, and as conferring uniqueness. Ironically, however, this uniqueness is only achieved through an incorporation of collective, classed understandings. The paper calls for a problematization of a normative and normalized middle-class location that is, I argue, given added legitimacy by a perceived decline in the significance of class its...

Malaria in the African highlands: past, present and future.

Abstract: Many of the first European settlers in Africa sought refuge from the heat and diseases of the plains by moving to the cool and salubrious highlands. Although many of the highlands were originally malaria free, there has been a progressive rise in the incidence of the disease over the last 50 years, largely as a consequence of agroforestry development, and it has been exacerbated by scarce health resources. In these areas of fringe transmission where the malaria pattern is unstable, epidemics may be precipitated by relatively subtle climatic changes. Since there is little immunity against the disease in these communities, outbreaks can be devastating, resulting in a substantial increase in morbidity and death among both children and adults. We present here the results obtained using a mathematical model designed to identify these epidemic-prone regions in the African highlands and the differences expected to occur as a result of projected global climate change. These highlands should be recognized as an area of special concern. We further recommend that a regional modelling approach should be adopted to assess the extent and severity of this problem and help improve disease surveillance and the quality of health care delivered in this unstable ecosystem.