997 resultados para Galaxies: star clusters: individual: 30 Doradus


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We are developing two-layered Yttrium Barium Copper Oxide (YBCO) thin film structures for energy efficient data links for superconducting electronics and present the results of their property measurements. High temperature superconductors (HTS) are advantageous for the implementation of energy-efficient cables interconnecting low temperature superconductor-based circuits and other cryogenic electronics circuits at higher temperature stages. The advantages of the HTS cables come from their low loss and low dispersion properties, allowing ballistic transfer of low power signals with very high bandwidth, low heat conduction and negligible inter-line crosstalk. The microstrip line cable geometry for typical materials is a two-layered film, in which the two superconducting layers are separated by an insulation layer with a minimized permittivity. We have made a proof of concept design of two YBCO films grown by pulsed laser deposition and then assembled into a sandwich with uniform insulating interlayer of tens of micrometers thick. We report on results obtained from such systems assembled in different ways. Structural and electromagnetic properties have been examined on individual films and on the corresponding sandwich composite. © 2013 IEEE.

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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

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Pós-graduação em Medicina Veterinária - FMVZ

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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

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Pós-graduação em Agronomia (Agricultura) - FCA

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A desnutrição, altamente prevalente em países em desenvolvimento, é um mau antigo que aflige a humanidade. Apresenta-se como um estado de deficiência alimentar, com déficit global de proteínas e calorias, provocando menor aporte de nutrientes às células. Alguns estudos têm mostrado evidências de interação entre desnutrição e estresse oxidativo, ocasionado pelo acúmulo de espécies reativas de oxigênio que causam danos à estrutura das biomoléculas em decorrência da desregulação entre a produção de oxidante e a depleção das defesas antioxidantes. Nesse estudo foi avaliada a utilização da farinha instantânea de amaranto adicionada de arroz na proporção de 30/70% como suplemento alimentar da dieta de base do paraense usada como modelo de indução da desnutrição experimental em ratos sobre o estresse oxidativo dos animais desnutridos comparados aos controles e aos tratados com a dieta suplementada. A dieta modelo de desnutrição (DBR-PA) foi confeccionada respeitando-se as quantidades dos alimentos consumidos rotineiramente pela população do Pará, segundo inquérito alimentar realizado na década de 70 por pesquisadores da Universidade Federal do Pará, enquanto que, a dieta utilizada como tratamento foi elaborada adicionando-se a DBRPA 30% da farinha de amaranto. As análises da composição centesimal e o perfil de aminoácidos foram realizados de acordo com as normas do Instituto Adolfo Lutz (1995) e por espectrofotometria atômica. A dieta controle foi utilizada na forma que é comercializada. Para realização do estudo utilizou-se animais no pós parto imediato de mães alimentadas na gestação com dieta controle para ratos (22% de proteínas), com peso mínimo de 6 g ao nascer. No pós parto imediato as ratas mães foram divididas em 3 grupos a saber: grupo controle (22% de proteínas); grupo desnutridos (DBR-PA contendo 7,8% de proteínas) grupo 3 tratados (DBR-PA+AA) suplementada com a farinha instantânea de amaranto contendo 11,33%). No pós desmame os animais foram separados e em gaiolas individuais receberam a dieta materna específica de cada grupo até os 60 dias de vida, quando foram sacrificados e realizada a coleta de sangue para as dosagens bioquímicas (colesterol total e frações, valores hemogramas (hematimetria, leucograma e plaquetas), níveis de peroxidação lipídica e atividade da catalase. Após a coleta do sangue os animais foram submetidos à exerese do fígado para posterior análise histopatológica. Os resultados revelaram que a dieta indutora da desnutrição é um modelo de desnutrição grave comum na região norte, é hipoproteica, normocalórica, com aminoácido limitante (metionina), promoveu perda de peso nos animais desde o período de aleitamento com acentuado perda de peso nas ratas mãe e nos filhotes aos desmame (21 dias), aos 28 e 60 dias de vida (p <0,05) quando comparados aos animais tratados com amaranto e aos controles. A dieta suplementada com a farinha extrusada de amaranto promoveu ganho de peso no período do aleitamento tanto nas ratas mães (p<0,05) como nos filhotes a partir do 14º dias de uso da mesma ( p<0,05), aos 21 dias (desmame)(p<0,05) aos 28 ( p< 0,05)e 60º dias de vida (p<0,05). Os animais desnutridos consumiram mais dieta em todos os momentos avaliados quando comparados aos tratados e controles (p<0,05). Não foi observada diferença entre os grupos nos valores bioquímicos de hematimetria, leucograma, plaquetas, colesterol total e frações. Os níveis de peroxidação lipídica não apresentaram diferença estatística entre os grupos. A atividade da catalase foi maior no grupo tratado com a suplementação da farinha de amaranto quando comparado aos desnutridos.Os animais tanto os tratados com amaranto como os desnutridos apresentaram esteatose hepática e processo inflamatório dos hepatócitos.O estudo mostrou que a desnutrição imposta não ocasionou estresse oxidativo, porém a diminuição da atividade da catalase nos animais desnutridos pode ter sido ocasionado pela diminuição da síntese da catalase.

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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

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PURPOSE: Describe hearing aid use by the elderly population in the city of São Paulo and identify associated factors. METHODS: A cross-sectional, descriptive, quantitative study integrated with the SABE (health, well-being and aging) project developed in 2006. A total of 1.115 individuals aged 65 or over were interviewed. Sample selection occurred in two stages, with replacement and probabilities proportional to the population to complement those aged 75 or over. Structured questionnaires and validated instruments were used. The data were weighted, the Rao-Scott test was used for univariate analysis and backward stepwise logistic regression was used for multivariate analysis, performed on Stata 10® software. RESULTS: Three hundred and seventy-seven subjects (30.4%) were classified as hearing impaired and 10.1% of these reported using hearing aids. To acquire the devices, 78.8% used their own resources and 16.9% acquired them through the Brazilian public health system (SUS). Among non-users of hearing aids, 16.6% reported prior indication; however, 8.6% were unable to adapt to the device and 8.0% could not afford to acquire one. Hearing aid use was associated with lower prevalence of probable dementia. CONCLUSION: The low number of hearing aid users indicates the difficulties elderly people face in acquiring them and/or that the health services face in effectively helping them to adapt. These findings may influence the quality of life of elderly with hearing impairment, given the association with probable dementia revealed by this study.

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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

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Pós-graduação em Zootecnia - FCAV

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The western spread of raccoon rabies in Alabama has been slow and even appears to regress eastward periodically. While the disease has been present in the state for over 30 years, areas in northwest Alabama are devoid of raccoon rabies. This variation resulting in an enzootic area of raccoon rabies primarily in southeastern Alabama may be due to landscape features that hinder the movement of raccoons (i.e., gene flow) among different locations. We used 11 raccoon-specific microsatellite markers to obtain individual genotypes to examine gene flow among areas that were rabies free, enzootic with rabies, or had only sporadic reports of the disease. Samples from 70 individuals were collected from 5 sampling localities in 3 counties. The landscape feature data were collected from geographic information system (GIS) data. We inferred gene flow by estimating FST and by using Bayesian tests to identify genetic clusters. Estimates of pairwise FST indicated genetic differentiation and restricted gene flow between some sites, and an uneven distribution of genetic clusters was observed. Of the landscape features examined (i.e., land cover, elevation, slope, roads, and hydrology), only land cover had an association with genetic differentiation, suggesting this landscape variable may affect gene flow among raccoon populations and thus the spread of raccoon variant of rabies in Alabama.

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We present a photometric catalogue of compact groups of galaxies (p2MCGs) automatically extracted from the Two-Micron All Sky Survey (2MASS) extended source catalogue. A total of 262 p2MCGs are identified, following the criteria defined by Hickson, of which 230 survive visual inspection (given occasional galaxy fragmentation and blends in the 2MASS parent catalogue). Only one quarter of these 230 groups were previously known compact groups (CGs). Among the 144 p2MCGs that have all their galaxies with known redshifts, 85 (59?per cent) have four or more accordant galaxies. This v2MCG sample of velocity-filtered p2MCGs constitutes the largest sample of CGs (with N = 4) catalogued to date, with both well-defined selection criteria and velocity filtering, and is the first CG sample selected by stellar mass. It is fairly complete up to Kgroup similar to 9 and radial velocity of similar to 6000?km?s-1. We compared the properties of the 78 v2MCGs with median velocities greater than 3000?km?s-1 with the properties of other CG samples, as well as those (mvCGs) extracted from the semi-analytical model (SAM) of Guo et al. run on the high-resolution Millennium-II simulation. This mvCG sample is similar (i.e. with 2/3 of physically dense CGs) to those we had previously extracted on three other SAMs run on the Millennium simulation with 125 times worse spatial and mass resolutions. The space density of v2MCGs within 6000?km?s-1 is 8.0 X 10-5?h3?Mpc-3, i.e. four times that of the Hickson sample [Hickson Compact Group (HCG)] up to the same distance and with the same criteria used in this work, but still 40?per cent less than that of mvCGs. The v2MCG constitutes the first group catalogue to show a statistically large firstsecond ranked galaxy magnitude gap according to TremaineRichstone statistics, as expected if the first ranked group members tend to be the products of galaxy mergers, and as confirmed in the mvCGs. The v2MCG is also the first observed sample to show that first-ranked galaxies tend to be centrally located, again consistent with the predictions obtained from mvCGs. We found no significant correlation of group apparent elongation and velocity dispersion in the quartets among the v2MCGs, and the velocity dispersions of apparently round quartets are not significantly larger than those of chain-like ones, in contrast to what has been previously reported in HCGs. By virtue of its automatic selection with the popular Hickson criteria, its size, its selection on stellar mass, and its statistical signs of mergers and centrally located brightest galaxies, the v2MCG catalogue appears to be the laboratory of choice to study physically dense groups of four or more galaxies of comparable luminosity.

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Knowing which individuals can be more efficient in spreading a pathogen throughout a determinate environment is a fundamental question in disease control. Indeed, over recent years the spread of epidemic diseases and its relationship with the topology of the involved system have been a recurrent topic in complex network theory, taking into account both network models and real-world data. In this paper we explore possible correlations between the heterogeneous spread of an epidemic disease governed by the susceptible-infected-recovered (SIR) model, and several attributes of the originating vertices, considering Erdos-Renyi (ER), Barabasi-Albert (BA) and random geometric graphs (RGG), as well as a real case study, the US air transportation network, which comprises the 500 busiest airports in the US along with inter-connections. Initially, the heterogeneity of the spreading is achieved by considering the RGG networks, in which we analytically derive an expression for the distribution of the spreading rates among the established contacts, by assuming that such rates decay exponentially with the distance that separates the individuals. Such a distribution is also considered for the ER and BA models, where we observe topological effects on the correlations. In the case of the airport network, the spreading rates are empirically defined, assumed to be directly proportional to the seat availability. Among both the theoretical and real networks considered, we observe a high correlation between the total epidemic prevalence and the degree, as well as the strength and the accessibility of the epidemic sources. For attributes such as the betweenness centrality and the k-shell index, however, the correlation depends on the topology considered.

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While the presence of discs around classical Be stars is well established, their origin is still uncertain. To understand what processes result in the creation of these discs and how angular momentum is transported within them, their physical properties must be constrained. This requires comparing high spatial and spectral resolution data with detailed radiative transfer modelling. We present a high spectral resolution, R similar to 80 000, sub-milliarcsecond precision, spectroastrometric study of the circumstellar disc around the Be star beta CMi. The data are confronted with 3D, non-local thermodynamic equilibrium radiative transfer calculations to directly constrain the properties of the disc. Furthermore, we compare the data to disc models featuring two velocity laws: Keplerian, the prediction of the viscous disc model, and angular momentum conserving rotation. It is shown that the observations of beta CMi can only be reproduced using Keplerian rotation. The agreement between the model and the observed spectral energy distribution, polarization and spectroastrometric signature of beta CMi confirms that the discs around Be stars are well modelled as viscous decretion discs.

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We present an analysis of observations made with the Arcminute Microkelvin Imager (AMI) and the CanadaFranceHawaii Telescope (CFHT) of six galaxy clusters in a redshift range of 0.160.41. The cluster gas is modelled using the SunyaevZeldovich (SZ) data provided by AMI, while the total mass is modelled using the lensing data from the CFHT. In this paper, we (i) find very good agreement between SZ measurements (assuming large-scale virialization and a gas-fraction prior) and lensing measurements of the total cluster masses out to r200; (ii) perform the first multiple-component weak-lensing analysis of A115; (iii) confirm the unusual separation between the gas and mass components in A1914 and (iv) jointly analyse the SZ and lensing data for the relaxed cluster A611, confirming our use of a simulation-derived masstemperature relation for parametrizing measurements of the SZ effect.