TOWARD UNDERSTANDING THE B[e] PHENOMENON. IV. MODELING OF IRAS 00470+6429

FS CMa type stars are a recently described group of objects with the B[e] phenomenon which exhibits strong emission-line spectra and strong IR excesses. In this paper, we report the first attempt for a detailed modeling of IRAS 00470+6429, for which we have the best set of observations. Our modeling is based on two key assumptions: the star has a main-sequence luminosity for its spectral type (B2) and the circumstellar (CS) envelope is bimodal, composed of a slowly outflowing disklike wind and a fast polar wind. Both outflows are assumed to be purely radial. We adopt a novel approach to describe the dust formation site in the wind that employs timescale arguments for grain condensation and a self-consistent solution for the dust destruction surface. With the above assumptions we were able to satisfactorily reproduce many observational properties of IRAS 00470+6429, including the Hi line profiles and the overall shape of the spectral energy distribution. Our adopted recipe for dust formation proved successful in reproducing the correct amount of dust formed in the CS envelope. Possible shortcomings of our model, as well as suggestions for future improvements, are discussed.

Searching for s-Process-Enhanced Metal-Poor Stars

We present preliminary results for the estimation of barium [Ba/Fe], and strontium [Sr/Fe], abundances ratios using medium-resolution spectra (1-2 angstrom). We established a calibration between the abundance ratios and line indices for Ba and Sr, using multiple regression and artificial neural network techniques. A comparison between the two techniques (showing the advantage of the latter), as well as a discussion of future work, is presented.

Global properties of `ordinary` early-type galaxies: photometry and spectroscopy of stars and globular clusters in NGC 4494

We present a comprehensive analysis of the spatial, kinematic and chemical properties of stars and globular clusters (GCs) in the `ordinary` elliptical galaxy NGC 4494 using data from the Keck and Subaru telescopes. We derive galaxy surface brightness and colour profiles out to large galactocentric radii. We compare the latter to metallicities derived using the near-infrared Calcium Triplet. We obtain stellar kinematics out to similar to 3.5 effective radii. The latter appear flattened or elongated beyond similar to 1.8 effective radii in contrast to the relatively round photometric isophotes. In fact, NGC 4494 may be a flattened galaxy, possibly even an S0, seen at an inclination of similar to 45 degrees. We publish a catalogue of 431 GC candidates brighter than i(0) = 24 based on the photometry, of which 109 are confirmed spectroscopically and 54 have measured spectroscopic metallicities. We also report the discovery of three spectroscopically confirmed ultra-compact dwarfs around NGC 4494 with measured metallicities of -0.4 less than or similar to [Fe/H] less than or similar to -0.3. Based on their properties, we conclude that they are simply bright GCs. The metal-poor GCs are found to be rotating with similar amplitude as the galaxy stars, while the metal-rich GCs show marginal rotation. We supplement our analysis with available literature data and results. Using model predictions of galaxy formation, and a suite of merger simulations, we find that many of the observational properties of NGC 4494 may be explained by formation in a relatively recent gas-rich major merger. Complete studies of individual galaxies incorporating a range of observational avenues and methods such as the one presented here will be an invaluable tool for constraining the fine details of galaxy formation models, especially at large galactocentric radii.

Metallicity gradients at large galactocentric radii using the near-infrared Calcium triplet

We describe a new spectroscopic technique for measuring radial metallicity gradients out to large galactocentric radii. We use the DEep Imaging Multi-Object Spectrograph (DEIMOS) on the Keck telescope and the galaxy spectrum extraction technique of Proctor et al. We also make use of the metallicity sensitive near-infrared Calcium ii triplet (CaT) features together with single stellar population models to obtain metallicities. Our technique is applied as a pilot study to a sample of three relatively nearby (< 30 Mpc) intermediate-mass to massive early-type galaxies. Results are compared with previous literature inner region values and generally show good agreement. We also include a comparison with profiles from dissipational disc-disc major merger simulations. Based on our new extended metallicity gradients combined with other observational evidence and theoretical predictions, we discuss possible formation scenarios for the galaxies in our sample. The limitations of our new technique are also discussed.

Probing the 2D kinematic structure of early-type galaxies out to three effective radii

We detail an innovative new technique for measuring the two-dimensional (2D) velocity moments (rotation velocity, velocity dispersion and Gauss-Hermite coefficients h(3) and h(4)) of the stellar populations of galaxy haloes using spectra from Keck DEIMOS (Deep Imaging Multi-Object Spectrograph) multi-object spectroscopic observations. The data are used to reconstruct 2D rotation velocity maps. Here we present data for five nearby early-type galaxies to similar to three effective radii. We provide significant insights into the global kinematic structure of these galaxies, and challenge the accepted morphological classification in several cases. We show that between one and three effective radii the velocity dispersion declines very slowly, if at all, in all five galaxies. For the two galaxies with velocity dispersion profiles available from planetary nebulae data we find very good agreement with our stellar profiles. We find a variety of rotation profiles beyond one effective radius, i.e. rotation speed remaining constant, decreasing and increasing with radius. These results are of particular importance to studies which attempt to classify galaxies by their kinematic structure within one effective radius, such as the recent definition of fast- and slow-rotator classes by the Spectrographic Areal Unit for Research on Optical Nebulae project. Our data suggest that the rotator class may change when larger galactocentric radii are probed. This has important implications for dynamical modelling of early-type galaxies. The data from this study are available on-line.

VELOCITY FIELD OF COMPRESSIBLE MAGNETOHYDRODYNAMIC TURBULENCE: WAVELET DECOMPOSITION AND MODE SCALINGS

We study compressible magnetohydrodynamic turbulence, which holds the key to many astrophysical processes, including star formation and cosmic-ray propagation. To account for the variations of the magnetic field in the strongly turbulent fluid, we use wavelet decomposition of the turbulent velocity field into Alfven, slow, and fast modes, which presents an extension of the Cho & Lazarian decomposition approach based on Fourier transforms. The wavelets allow us to follow the variations of the local direction of the magnetic field and therefore improve the quality of the decomposition compared to the Fourier transforms, which are done in the mean field reference frame. For each resulting component, we calculate the spectra and two-point statistics such as longitudinal and transverse structure functions as well as higher order intermittency statistics. In addition, we perform a Helmholtz-Hodge decomposition of the velocity field into incompressible and compressible parts and analyze these components. We find that the turbulence intermittency is different for different components, and we show that the intermittency statistics depend on whether the phenomenon was studied in the global reference frame related to the mean magnetic field or in the frame defined by the local magnetic field. The dependencies of the measures we obtained are different for different components of the velocity; for instance, we show that while the Alfven mode intermittency changes marginally with the Mach number, the intermittency of the fast mode is substantially affected by the change.

Regulation of Multidrug Resistance-Associated Protein 2 by Calcium Signaling in Mouse Liver

Mu hiding resistance associated protein 2 (Mrp2) is a canalicular transporter responsible for organic anion secretion into bile. Mrp2 activity is regulated by insertion into the plasma membrane; however, the factors that control this are not understood. Calcium (Ca(2+)) signaling regulates exocytosis of vesicles in most cell types, and the type II inositol 1,4,5-triphosphate receptor (InsP(3)R2) regulates Ca(2+) release in the canalicular region of hepatocytes. However, the role of InsP(3)R2 and of Ca(2+) signals in canalicular insertion and function of Mrp2 is not known. The aim of this study was to determine the role of InsP(3)R2-mediated Ca(2+) signals in targeting Mrp2 to the canalicular membrane. Livers, isolated hepatocytes, and hepatocytes in collagen sandwich culture from wild-type (WT) and InsP(3)R2 knockout (KO) mice were used for western blots, confocal immunofluorescence, and time-lapse imaging of Ca(2+) signals and of secretion of a fluorescent organic anion. Plasma membrane insertion of green fluorescent protein (GFP)-Mrp2 expressed in HepG2 cells was monitored by total internal reflection microscopy. InsP(3)R2 was concentrated in the canalicular region of WT mice but absent in InsP(3)R2 KO livers, whereas expression and localization of InsP(3)R1 was preserved, and InsP(3)R3 was absent from both WT and KO livers. Ca(2+) signals induced by either adenosine triphosphate (ATP) or vasopressin were impaired in hepatocytes lacking InsP(3)R2. Canalicular secretion of the organic anion 5-chloromethylfluorescein diacetate (CMFDA) was reduced in KO hepatocytes, as well as in WT hepatocytes treated with 1,2-bis(o-aminophenoxy)ethane-N,N,N`,N`-tetra-acetic acid (BAPTA). Moreover, the choleretic effect of tauroursodeoxycholic acid (TUDCA) was impaired in InsP(3)R2 KO mice. Finally, ATP increased GFP-Mrp2 fluorescence in the plasma membrane of HepG2 cells, and this also was reduced by BAPTA. Conclusion: InsP(3)R2-mediated Ca(2+) signals enhance organic anion secretion into bile by targeting Mrp2 to the canalicular membrane. (HEPATOLOGY 2010;52:327-337)

Acute toxicity of a single gavage dose of fumonisin B(1) in rabbits

The aim of this study was to determine the clinical, pathological and mycotoxicological effects of oral administration of fumonisin B, (FBI) in rabbits. Eighteen rabbits were randomly assigned to two experimental groups: control group, 0 mg FB(1): fumonisin group. 31.5 mg FB(1)/kg body weight, corresponding to about 630 mg FB(1)/kg diet. Fumonisin administered as a single oral dose to rabbits resulted in acute toxicity, significantly interfering with body and liver weight. Serum biochemical analysis revealed a significant increase of total protein, alkaline phosphatase (AP), aspartate aminotransferase (AST), alanine aminotransferase (ALT), gamma-glutamyltransferase (GGT), urea and creatinine in the group receiving FBI compared to control animals, a finding characterizing hepatic and renal injury in this group. Urinary protein concentrations were markedly elevated at 12,24,48 and 72 h after dosing, although visible pathological abnormalities were not observed, probably because of rapid repair of the damage. FBI was detected in feces, with a maximum concentration at 24h after administration, indicating that the enterohepatic circulation is important in rabbits. FBI concentrations found in urine were low, with peak elimination at 12 h after intoxication. The highest FBI concentrations were observed in feces compared to urine and liver, demonstrating that feces are the main routes of excretion. (C) 2009 Elsevier Ireland Ltd. All rights reserved.

A characterisation of the Hoffman-Wohlgemuth surfaces in terms of their symmetries

For an embedded singly periodic minimal surface (M) over tilde with genus rho >= 4 and annular ends, some weak symmetry hypotheses imply its congruence with one of the Hoffman-Wohlgemuth examples. We give a very geometrical proof of this fact, along which they come out many valuable clues for the understanding of these surfaces.

Relação entre a cultura organizacional e os indicadores de desempenho econômico, ambiental, e social de sustentabilidade do triple bottom line (3BL): um estudo nas companhias de energia elétrica

Tese apresentada ao Programa de Pós-Graduação em Administração da Universidade Municipal de São Caetano do Sul para obtenção do título de Doutora em Administração

Utilização da frutose-1, 6-Bisfosfato como um protetor celular na preservação de fígados para transplante

A solução de preservação da Universidade de Wisconsin (UW) é considerada a solução padrão para preservação de fígados, rins e pâncreas. A frutose-1,6-bisfosfato (FBP) é uma substância que apresenta efeito protetor do fígado contra injúrias provocadas por agentes químicos e ocorridas durante o período de isquemia-reperfusão. O objetivo deste estudo foi avaliar os efeitos da FBP na composição de soluções para preservação de fígados para transplante. Neste estudo experimental, a perfusão e a preservação dos fígados foram realizadas em cada grupo com as soluções de UW, UW contendo 10 mmol/L de FBP (UWM) e FBP 10 mmol/L (FBPS), respectivamente. Os fígados foram armazenados em um recipiente plástico contendo solução de preservação a 4oC por 24 horas. As mensurações bioquímicas de AST, ALT, LDH e TBARS foram realizadas em amostras das soluções de preservação nos tempos de 0, 12, 18 e 24 horas. A análise histológica foi realizada em fígados preservados por 24 horas. O grau de preservação observado com as soluções de UW e FBPS foi similar até 18 horas de armazenamento. A adição de 10 mmol/L de FBP à solução de UW provocou um aumento das injúrias ocorridas e uma pior preservação quando comparado ao grupo armazenado em UW. A FBP protegeu os fígados contra danos causados pelos radicais livres por tempos de preservação inferiores a 18 horas. Não houve diferença significativa entre os grupos na análise histológica dos fígados preservados no tempo de 24 horas. A FBP utilizada em solução foi eficaz na preservação de fígados, podendo ser um importante constituinte para outras formulações.

Contribuição ao estudo das hepatectomias parciais com oclusão do fluxo sanguíneo aferente

O tratamento cirúrgico dos tumores hepáticos tem sido um grande desafio na história evolutiva da cirurgia. No passado, as altas taxas de morbidade e mortalidade limitavam sua aplicação como opção terapêutica. O refinamento da técnica de ressecção hepática está associado a menores índices de mortalidade e morbidade peri-operatória e, embora, a mortalidade tenha sido reduzida a menos de 10% nos serviços especializados, a morbidade ainda é bastante significativa, sendo que a hemorragia grave e a embolia aérea permanecem como complicações graves das hepatectomias. O controle da perda sanguínea é o objetivo primordial durante este tipo de cirurgia. As técnicas descritas, com a finalidade de conter a hemorragia transoperatória, são aquelas associadas à redução do fluxo sanguíneo ao fígado, seja através da oclusão vascular aferente ou manobra de Pringle por clampeamento do pedículo hepático, seja por exclusão vascular total do órgão. Hepatectomias parciais podem ser realizadas com pequeno sangramento e, mesmo quando associadas a períodos prolongados de isquemia tecidual, não foram identificadas lesões parenquimatosas ou falência hepática persistente. A redução na necessidade de reposição de sangue, no período peri-operatório, está associada a menor morbidade e à diminuição significativa na incidência de sepse abdominal. O objetivo deste estudo foi o de avaliar uma série de hepatectomias parciais com oclusão do fluxo sanguíneo aferente, em pacientes portadores de patologias benignas e neoplasias malignas. Foram analisadas 60 hepatectomias em 59 pacientes com oclusão do fluxo sanguíneo aferente quanto a possíveis fatores de risco para morbidade e mortalidade, bem como a relação entre o tempo de isquemia hepática e a variação das transaminases, tempo de protrombina e bilirrubinas, e destes, com a evolução pós-operatória. A prevalência de complicações pós-operatórias foi de 43,3% e a mortalidade de 6,7%. O fator de risco significativo para mortalidade foi tempo cirúrgico mais prolongado, quando comparado com os pacientes que não foram a óbito. Para a morbidade pós-operatória, foram identificados como fatores de risco a idade acima de 60 anos, cirurgia por neoplasia maligna, parênquima hepático anormal, ou seja, presença de cirrose, esteatose ou colestase, perda sanguínea necessitando reposição de mais de uma unidade de sangue e outros procedimentos cirúrgicos concomitantes. Na análise multivariada por regressão logística, estes fatores de risco foram reduzidos, apenas, para presença de cirrose, esteatose ou colestase. O tempo de isquemia não apresentou relação com a morbi-mortalidade pós-operatória. A variação das transaminases foram mais acentuadas nos casos com maior tempo de isquemia, porém, retornaram aos níveis pré-operatórios em, aproximadamente, uma semana. Não houve variação de tempo de protrombina e bilirrubinas quanto ao tempo de isquemia. A variação de AST e ALT não foram diferentes entre os pacientes com e sem morbidade pós-operatória.

O método de Perron : aplicações e extensões

Nesta dissertação apresentamos e desenvolvemos o Método de Perron, fazendo uma aplicação ao ploblema de Dirichlet para a equação das superfícies de curvatura média constante em R3. Apresentamos também uma extensão deste método dentro de EDP's e, por fim, obtemos uma extensão geométrica que se aplica a superfícies ao invés de gráficos. Comentamos a aplicação deste método geométrico á existência de superfícies mínimas tendo como bordo duas curvas convexas em planos paralelos do R3.