Turning waves and breakdown for incompressible flows

We consider the evolution of an interface generated between two immiscible incompressible and irrotational fluids. Specifically we study the Muskat and water wave problems. We show that starting with a family of initial data given by (\al,f_0(\al)), the interface reaches a regime in finite time in which is no longer a graph. Therefore there exists a time $t^*$ where the solution of the free boundary problem parameterized as (\al,f(\al,t)) blows-up: \|\da f\|_{L^\infty}(t^*)=\infty. In particular, for the Muskat problem, this result allows us to reach an unstable regime, for which the Rayleigh-Taylor condition changes sign and the solution breaks down.Comment: 15 page

1.3 mm Polarized emission in the circumstellar disk of a massive protostar

We present the first resolved observations of the 1.3 mm polarized emission from the disk-like structure surrounding the high-mass protostar Cepheus A HW2. These CARMA data partially resolve the dust polarization, suggesting a uniform morphology of polarization vectors with an average position angle of 57° ± 6° and an average polarization fraction of 2.0% ± 0.4%. The distribution of the polarization vectors can be attributed to (1) the direct emission of magnetically aligned grains of dust by a uniform magnetic field, or (2) the pattern produced by the scattering of an inclined disk. We show that both models can explain the observations, and perhaps a combination of the two mechanisms produces the polarized emission. A third model including a toroidal magnetic field does not match the observations. Assuming scattering is the polarization mechanism, these observations suggest that during the first few 104 years of high-mass star formation, grain sizes can grow from1 mm to several 10s μm.Fil: Fernandez Lopez, Manuel. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaFil: Stephens, I. W.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Boston University; Estados Unidos. University of Illinois; Estados UnidosFil: Girart, J. M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Institut de Ciències de l’Espai; EspañaFil: Looney, L.. University of Illinois; Estados UnidosFil: Curiel, S.. Universidad Nacional Autónoma de México; MéxicoFil: Segura Cox, D.. University of Illinois; Estados UnidosFil: Eswaraiah, C.. National Tsing Hua University; República de ChinaFil: Lai, S. P.. National Tsing Hua University; República de Chin

Lista de los peces de la provincia de Santiago del Estero

…los censos de la fauna de un país o región cualquiera, constituyen una suerte de codificación de la Naturaleza, como paso previo e indispensable para un ensayo racional de aprovechamiento de las riquezas naturales y de su adecuada conservación. Desde fines del siglo XVIII se ha dicho, y lo han repetido en nuestro medio, Cosme Argerich, Alberto Palcos y otros estudiosos y cientistas, que un Código de la Naturaleza es indispensable para la libertad de una nación. [R. A. Ringuelet & R. H. Arámburu. Enumeración sistemática de los vertebrados de la Provincia de Buenos Aires. La Plata, MAA, Publ. 119, 1957].Fil: Fernandez, Luis Alfredo. Fundación Miguel Lillo; Argentina. Universidad Nacional de Catamarca. Facultad de Ciencias Exactas y Naturales; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Nadalin, D.. Universidad Nacional de La Plata. Facultad de Ciencias Naturales y Museo; ArgentinaFil: Lopez, H. L.. Universidad Nacional de La Plata. Facultad de Ciencias Naturales y Museo; ArgentinaFil: Andreoli Bize, M. J.. Universidad Nacional de Catamarca. Facultad de Ciencias Exactas y Naturales; Argentin

Stick-slip instabilities in the shear flow of magnetorheological suspensions

International audienceThis work is devoted to the stick-slip instabilities that appear in the shear flow of highly concentrated suspensions of magnetic microparticles. The effect of the applied magnetic field strength was analyzed in details. With this aim, homogeneous suspensions of iron microparticles with concentration near the limit of maximum-packing fraction were prepared, and shear-flow measurements were performed in a controlled-rate mode using a rheometer provided with a rough parallel-plate geometry. For each given value of the shear rate, the time evolution of the shear stress was monitored for at least 20 min. Saw-tooth-like stress oscillations, typical of stick-slip instabilities, were obtained at low enough shear rate values. The measurements were restricted to small enough oscillations, at which the rheometer was still able to maintain the shear rate constant. From the microscopic viewpoint, these stick-slip instabilities principally appear due to the periodic failure and healing of the field-induced particle structures, as inferred from experimental observations. This hypothesis is corroborated by a theoretical model developed on the basis of the balance of the magnetic and hydrodynamic torques over the particle structures, allows us to predict the correct order of magnitude of the main parameters of the stick-slip instabilities, including the amplitude and period of the stress oscillations

Resolving galaxies in time and space: II: Uncertainties in the spectral synthesis of datacubes

In a companion paper we have presented many products derived from the application of the spectral synthesis code STARLIGHT to datacubes from the CALIFA survey, including 2D maps of stellar population properties and 1D averages in the temporal and spatial dimensions. Here we evaluate the uncertainties in these products. Uncertainties due to noise and spectral shape calibration errors and to the synthesis method are investigated by means of a suite of simulations based on 1638 CALIFA spectra for NGC 2916, with perturbations amplitudes gauged in terms of the expected errors. A separate study was conducted to assess uncertainties related to the choice of evolutionary synthesis models. We compare results obtained with the Bruzual & Charlot models, a preliminary update of them, and a combination of spectra derived from the Granada and MILES models. About 100k CALIFA spectra are used in this comparison. Noise and shape-related errors at the level expected for CALIFA propagate to 0.10-0.15 dex uncertainties in stellar masses, mean ages and metallicities. Uncertainties in A_V increase from 0.06 mag in the case of random noise to 0.16 mag for shape errors. Higher order products such as SFHs are more uncertain, but still relatively stable. Due to the large number statistics of datacubes, spatial averaging reduces uncertainties while preserving information on the history and structure of stellar populations. Radial profiles of global properties, as well as SFHs averaged over different regions are much more stable than for individual spaxels. Uncertainties related to the choice of base models are larger than those associated with data and method. Differences in mean age, mass and metallicity are ~ 0.15 to 0.25 dex, and 0.1 mag in A_V. Spectral residuals are ~ 1% on average, but with systematic features of up to 4%. The origin of these features is discussed. (Abridged)Comment: A&A, accepte

On the MBM12 Young Association

I present a comprehensive study of the MBM12 young association (MBM12A). By combining infrared (IR) photometry from the Two-Micron All-Sky Survey (2MASS) survey with new optical imaging and spectroscopy, I have performed a census of the MBM12A membership that is complete to 0.03 Msun (H~15) for a 1.75deg X 1.4deg field encompassing the MBM12 cloud. I find five new members with masses of 0.1-0.4 Msun and a few additional candidates that have not been observed spectroscopically. From an analysis of optical and IR photometry for stars in the direction of MBM12, I identify M dwarfs in the foreground and background of the cloud. By comparing the magnitudes of these stars to those of local field dwarfs, I arrive at a distance modulus 7.2+/-0.5 (275 pc) to the MBM12 cloud; it is not the nearest molecular cloud and is not inside the local bubble of hot ionized gas as had been implied by previous distance estimates of 50-100 pc. I have also used Li strengths and H-R diagrams to constrain the absolute and relative ages of MBM12A and other young populations; these data indicate ages of 2 +3/-1 Myr for MBM12A and 10 Myr for the TW Hya and Eta Cha associations. MBM12A may be a slightly evolved version of the aggregates of young stars within the Taurus dark clouds (~1 Myr) near the age of the IC 348 cluster (~2 Myr).Comment: to be published in The Astrophysical Journal, 41 pages, 14 figures, also found at http://cfa-www.harvard.edu/sfgroup/preprints.htm

Adiponectina iria determinar o predomínio de VLDL alteradas na síndrome metabólica

El objetivo del trabajo fue evaluar si la reducción de adiponectina (ADP) en el síndrome metabólico (SMet), influencia las características aterogénicas de VLDL. Se estudiaron 45 pacientes con SMet y 15 controles sanos. En suero en ayunas se midió perfil lipídico, ácidos grasos libres (AGL), ADP, se aisló VLDL (d<1,006 g/L) caracterizándola en su composición química y tamaño (HPLC-exclusión molecular). En plasma post-heparínico se determinó la actividad de lipoproteína lipasa (LPL). En SMet VLDL mostró incremento de masa, número de partículas, contenido en triglicéridos-VLDL y mayor proporción de VLDL grandes (p<0,05). El incremento de AGL correlacionó con la masa de VLDL (r=0,36; p=0,009), número de partículas-VLDL (r=0,45; p=0,0006) y %-VLDL grandes (r=0,32; p=0,02). SMet mostró descenso en ADP (7,4±4,8 vs.15,5±7,2 μg/mL, p=0,01) y en actividad de LPL (p=0,01), que correlacionaron entre si (r=0,38; p=0,01; ajustado por HOMA-IR y cintura: β=0,35; p=0,02).ADP correlacionó negativamente con AGL y %-VLDL grandes (p<0,03). Se concluye que en SMet la disminución de ADP favorecería la secreción de VLDL sobre-enriquecidas en triglicéridos y de mayor tamaño, y además retardaría el catabolismo de VLDL mediado por LPL, resultando en la acumulación de VLDL alteradas en circulación con características aterogénicas.The aim of the work was to evaluate whether the reduction of adiponectin (ADP) in metabolic syndrome (MetS) affects the atherogenic features of VLDL. A total of 45 patients with MetS (ATPIII) and 15 healthy controls were studied. In fasting serum, lipid profile, free fatty acids (FFA) and ADP were determined. VLDL was isolated (d<1.006 g/L) and characterized in chemical composition and size (size exclusion-HPLC). In post-heparin plasma, lipoprotein lipase (LPL) activity was measured. In MetS, VLDL showed increased total mass, particle number, VLDL-triglyceride content and higher large-VLDL proportion (p<0.05). The increase in FFA correlated with VLDL mass (r=0.36; p=0.009), VLDL particle number (r=0.45; p=0.0006) and large-VLDL proportion (r=0.32; p=0.02). MetS patients showed a decrease in ADP (7.4±4.8 vs. 15.5±7.2 μg/mL, p=0.01) and in LPL activity (p=0.01), that positively correlated between them (r=0.38; p=0.01; adjusted by HOMA-IR and waist: β=0.35; p=0.02). ADP inversely correlated with FFA and large-VLDL% (p<0.03). It can be concluded that in MetS, decreased ADP would favour the secretion of triglyceride over-enriched and larger VLDL particles, and also would delay VLDL catabolism mediated by LPL, resulting in the accumulation of altered VLDL with atherogenic characteristics.O objetivo do trabalho foi avaliar se a redução da adiponectina (ADP) na síndrome metabólica (SM), afeta as características aterogênicas das VLDL. Foram estudados 45 indivíduos com SM e 15 controles saudáveis. Em jejum, foi medido em soro o perfil lipídico, ácidos graxos livres (AGL) e ADP. Foram isoladas as VLDL (d <1,006 g / L) caracterizando-as em relação a sua composição química e tamanho (HPLC- exclusão molecular). No plasma pós-heparina foi medida a atividade da lipoproteína lipase (LPL). Em indivíduos com SM, as VLDL apresentaram aumento de massa, número de partículas, conteúdo de triglicerídeos -VLDL e maior proporção de VLDL grandes (p<0,05). O aumento de AGL correlacionou com a massa de VLDL (r=0,36; p=0,009), número de partículas -VLDL (r=0,45; p=0,0006) e percentual -VLDL grandes (r=0,32; p=0,02). A SM mostrou uma diminuição em ADP (7,4±4,8 vs. 15,5±7,2 μg/mL, p=0,01) e em atividade de LPL (p=0,01), que correlacionaram entre eles (r=0,38; p=0,01; ajustada por HOMA-IR e cintura: β=0,35; p=0,02). A ADP correlacionou em forma negativa com AGL e %-VLDL grandes (p<0,03). A conclusão é que em indivíduos com SM, a diminuição da ADP iria favorecer a secreção de VLDL super-enriquecidas em triglicerídeos e de maior tamanho, e também atrasaria o catabolismo das VLDL mediado por LPL, resultando na acumulação de VLDL alteradas em circulação com características aterogênicas.Fil: Lucero, Diego Martín. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; ArgentinaFil: Miksztowicz, Verónica Julieta. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; ArgentinaFil: Cacciagiú, Leonardo D.. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; ArgentinaFil: Lopez, Graciela Ines. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; ArgentinaFil: Fernandez Machulsky, Nahuel Hernan. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; ArgentinaFil: Berg, Gabriela Alicia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; ArgentinaFil: Zago, Valeria. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; ArgentinaFil: Schreier, Laura Ester. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad de Buenos Aires. Facultad de Farmacia y Bioquímica. Departamento de Bioquímica Clínica; Argentin