1,860 research outputs found

    Human Rights and Post-War Reconstruction: Introduction

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    The expression “post-war reconstruction,” commonly adopted by both practitioners and academics, is somewhat misleading. Reconstruction does not entail rebuilding or return to the pre– war state of affairs as the expression seems to suggest. Rather, reconstruction involves difficult multiple transitions: from war to peace, from a state to a market economy, and from authoritarianism to democracy. Each transition taken by itself would be daunting. Taken together, they can be almost overwhelming

    Quasi-Periodic Variability in NGC 5408 X-1

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    We report the discovery with XMM-Newton of quasiperiodic variability in the 0.2 - 10 keV X-ray flux from the ultraluminous X-ray source NGC 5408 X-1. The average power spectrum of all EPIC-pn data reveals a strong 20 mHz QPO with an average amplitude (rms) of 9%, and a coherence of Q~6. In a 33 ksec time interval when the 20 mHz QPO is strongest we also find evidence for a 2nd QPO peak at 15 mHz. This is the first indication for a close pair of QPOs in a ULX source. Interestingly, the frequency ratio of this QPO pair is inconsistent with 3:2 at the 3sigma level, but is consistent with a 4:3 ratio. A powerlaw noise component with slope near 1.5 is also present below 0.1 Hz with evidence for a break to a flatter slope at about 3 mHz. The source shows substantial broadband variability, with a total amplitude (rms) of about 30% in the 0.1 - 100 mHz frequency band, and there is strong energy dependence to the variability. We discuss the implications of these findings in the context of models for ULXs, and their implications for the object's mass.Comment: 23 pages, 7 figures. Accepted for publication in the Astrophysical Journa

    Hermetia illucens and Poultry by-Product Meals as Alternatives to Plant Protein Sources in Gilthead Seabream (Sparus aurata) Diet: A Multidisciplinary Study on Fish Gut Status

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    The attempt to replace marine-derived ingredients for aquafeed formulation with plant-derived ones has met some limitations due to their negative side effects on many fish species. In this context, finding new, sustainable ingredients able to promote fish welfare is currently under exploration. In the present study, poultry by-products and Hermetia illucens meal were used to replace the vegetable protein fraction in diets totally deprived of fish meal intended for gilthead seabream (Sparus aurata). After a 12-week feeding trial, a multidisciplinary approach including histological, molecular, and spectroscopic techniques was adopted to investigate intestine and liver responses to the different dietary formulations. Regardless of the alternative ingredient used, the reduction in dietary vegetable proteins resulted in a lower incidence of intestine histological alterations and inflammatory responses. In addition, the dietary inclusion of insect meal positively affected the reduction in the molecular inflammatory markers analyzed. Spectroscopic analyses showed that poultry by-product meal improved lipid absorption in the intestine, while insect meal induced increased liver lipid deposition in fish. The results obtained demonstrated that both poultry by-products and H. illucens meal can successfully be used to replace plant-derived ingredients in diets for gilthead seabream, promoting healthy aquaculture

    The elusiveness of old neutron stars

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    Old neutron stars (ONSs) which have radiated away their internal and rotational energy may still shine if accreting the interstellar medium. Despite their large number, only two promising candidates have been detected so far and rather stringent limits on their observability follow from the analysis of ROSAT surveys. This contrasts with optimistic theoretical estimates that predicted a large number of sources in ROSAT fields. We have reconsidered the issue of ONSs observability, accounting for the spin and magnetic field evolution over the neutron star lifetime. In the framework of a spin-induced field decay model, we show that the total number of ONSs which are, at present, in the accretion stage is reduced by a factor ~5 over previous figures if the characteristic timescale for crustal current dissipation is ~ 10^8 - 10^9 yr. This brings theoretical predictions much closer to observational limits. Most ONSs should be at present in the propeller phase and, if subject to episodic flaring, they could be observable.Comment: 10 pages Latex, 5 ps figures. To be formatted with the AASTeX package. Accepted for publication in Ap

    Towards the Identification of a Suitable Commercial Diet for Carpione (Salmo carpio, Linnaeus 1758): A Multidisciplinary Study on Fish Performances, Animal Welfare and Quality Traits

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    SIMPLE SUMMARY: Carpione (Salmo carpio, Linnaeus 1758) is an endangered precious endemism of Lake Garda (Northern Italy), the largest Italian lake. To date, several bottlenecks about its culture remain unsolved, including the identification of a proper growth-out diet. In the present study, four different grossly isolipidic, isoproteic, and isoenergetic diets containing ingredients from different origins were used for S. carpio culture. Specifically, a diet largely based on marine ingredients, and currently used for carpione farming, was used as control. Three other diets were formulated in order to include relevant percentages of vegetable ingredients or processed animal proteins (at two different inclusion levels). After a three-month feeding trial, fish zootechnical performances, welfare, and flesh quality were evaluated through a multidisciplinary approach, including histology, gene expression, chemical analysis, and Fourier transform infrared spectroscopy (FTIR). This study provided the first insights on carpione physiological responses to different commercial dietary formulations. ABSTRACT: Carpione (Salmo carpio, Linnaeus 1758) is an endangered precious endemism of Lake Garda (Northern Italy), the largest Italian lake. To date, several bottlenecks about its culture remain unsolved, including the identification of a proper growth-out diet. The aim of the present study was to test four different grossly isolipidic, isoproteic, and isoenergetic diets in which the main ingredients had a different origin. Specifically, a diet currently used by local farmers for carpione culture, largely based on marine ingredients, was used as control (CTRL), while the other three diets were formulated by partially replacing marine ingredients with plant ones (VEG) or with different percentages of processed animal proteins (PAP1 and PAP2). The feeding trial was run in triplicate, over a three-month period. No significant differences in growth performance among the experimental groups were observed. However, remarkable histological alterations and inflammatory markers upregulation were observed in VEG group, while PAP inclusion played a role in attenuating inflammation and improving nutrient uptake. Fillet analyses highlighted significant differences in marketable traits and flesh fatty acid composition among the experimental groups, including the reduction of polyunsaturated fatty acids related to PAPs inclusion. In conclusion, PAPs used in the present study promoted S. carpio gut health and absorption capacity, while further studies are required to maintain proper quality traits of the final product

    Resolved, expanding jets in the Galactic black hole candidate XTE J1908+094

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    Black hole X-ray binaries undergo occasional outbursts caused by changing inner accretion flows. Here we report high angular resolution radio observations of the 2013 outburst of the black hole candidate X-ray binary system XTE J1908+094, using data from the Very Long Baseline Array and European VLBI Network. We show that following a hard-to-soft state transition, we detect moving jet knots that appear asymmetric in morphology and brightness, and expand to become laterally resolved as they move away from the core, along an axis aligned approximately −11° east of north. We initially see only the southern component, whose evolution gives rise to a 15-mJy radio flare and generates the observed radio polarization. This fades and becomes resolved out after 4 days, after which a second component appears to the north, moving in the opposite direction. From the timing of the appearance of the knots relative to the X-ray state transition, a 90° swing of the inferred magnetic field orientation, the asymmetric appearance of the knots, their complex and evolving morphology, and their low speeds, we interpret the knots as working surfaces where the jets impact the surrounding medium. This would imply a substantially denser environment surrounding XTE J1908+094 than has been inferred to exist around the microquasar sources GRS 1915+105 and GRO J1655−40

    Revisiting the ultraluminous supersoft source in M 101: An optically thick outflow model

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    The M 101 galaxy contains the best-known example of an ultraluminous supersoft source (ULS), dominated by a thermal component at kT ≈ 0.1 keV. The origin of the thermal component and the relation between ULSs and standard (broad-band spectrum) ultraluminous X-ray sources are still controversial. We re-examined the X-ray spectral and timing properties of the M 101 ULS using archival Chandra and XMM–Newton observations. We show that the X-ray time-variability and spectral properties are inconsistent with standard-disc emission. The characteristic radius Rbb of the thermal emitter varies from epoch to epoch between ≈10 000 and ≈100 000 km; the colour temperature kTbb varies between ≈50 and ≈140 eV and the two quantities scale approximately as R bb ∝T −2 bb Rbb∝Tbb−2. In addition to the smooth continuum, we also find (at some epochs) spectral residuals well fitted with thermal-plasma models and absorption edges: we interpret this as evidence that we are looking at a clumpy, multitemperature outflow. We suggest that at sufficiently high accretion rates and inclination angles, the supercritical, radiatively driven outflow becomes effectively optically thick and completely thermalizes the harder X-ray photons from the inner part of the inflow, removing the hard spectral tail. We develop a simple, spherically symmetric outflow model and show that it is consistent with the observed temperatures, radii and luminosities. A larger, cooler photosphere shifts the emission peak into the far-UV and makes the source dimmer in X-rays but possibly ultraluminous in the UV. We compare our results and interpretation with those of Liu et al

    SERVIÇOS E PRODUTOS DO SIBi/USP: descrição dos processos essenciais, gerenciais e de apoio

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    O Modelo de Gestão do Sistema Integrado de Bibliote\ud cas da Universidade de São Paulo\ud (SIBi/USP) incorpora conceitos e ferramentas de ger\ud enciamento que permeiam as\ud organizações modernas para garantir melhores índice\ud s de desempenho sistêmico e prestar\ud serviços com qualidade e eficiência aos usuários. C\ud omo parte do Modelo está a\ud identificação e a descrição detalhada dos processos\ud de trabalho do Sistema, assim como o\ud estabelecimento de alguns indicadores de desempenho\ud . A partir do\ud trabalho inicial, foi\ud elaborado um levantamento complementar para identif\ud icação dos processos que\ud abrangessem o conjunto do Sistema de forma ampla. O\ud s dados foram dispostos em\ud planilhas para melhor visualização, especialmente q\ud uanto aos macro processos, processos,\ud sub processos e atividades. Os processos foram sepa\ud rados em essenciais, gerenciais e de\ud apoio, além de elencadas as atividades pertinentes\ud a cada um deles, bem como as\ud instruções técnicas e fluxos de trabalho. Foram est\ud abelecidos alguns indicadores, tendo por\ud referência os da IFLA já estudados por outro Grupo\ud de Trabalho. Daquele estudo quatro\ud indicadores foram testados e validados pelo SIBi/US\ud P por meio de aplicação piloto em\ud algumas das Bibliotecas do Sistema e outros foram d\ud efinidos no estudo atual. Com isso foi\ud possível mapear os processos e as atividades desenv\ud olvidas pelo conjunto de Bibliotecas\ud sendo que cada Biblioteca, em função de sua especia\ud lidade e especificidade pode adequar\ud o seu mapeamento. A definição de um núcleo básico d\ud e indicadores objetiva viabilizar a\ud concretização da missão e dos objetivos em consonân\ud cia com a política do SIBI/USPThe Management Model of the Integrated Library Syst\ud em, University of São Paulo\ud (SIBi/USP) incorporates concepts and management too\ud ls that permeate modern\ud organizations to ensure better systemic performance\ud indexes and provide services\ud with quality and efficiency to users. Is part of th\ud e model, the identification and the\ud detailed description of the essential processes, ma\ud nagement and support, as well as\ud the establishment of some performance indicators. F\ud rom the initial work, we designed\ud a complementary survey to identify the processes co\ud vering the whole of the System.\ud Data were arranged in sheets for easy viewing, espe\ud cially with regard to macro \ud processes, processes, sub processes and activities.\ud The processes were divided into\ud essential, managerial and support. At that time, we\ud re listed the activities under each\ud processes and their technical instructions and work\ud flows. It were established some\ud indicators, using model IFLA already studied by oth\ud er Working Group. In this study\ud four indicators have been tested and validated by S\ud IBi/USP through pilot application\ud in some of the Library System and others were defin\ud ed in the current study. It was\ud possible to map the processes and activities undert\ud aken by all Libraries of SIBi/USP,\ud and each of them, depending on their specialty and\ud specificity can do its own\ud mapping. The definition of a core of indicators can\ud enable the achievement of the\ud mission and objectives in line with the policy of S\ud IBI/US
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