1,151 research outputs found

    Réhabilitation immunonutritionnelle d'enfants atteints de malnutrition sévère

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    Le déficit immunitaire de l'enfant souffrant de malnutrition est connu de longue date mais rarement pris en compte dans le processus de récupération nutritionnelle. Le centre de réhabilitation immunonutritionnelle (CRIN) de Cochabamba (Bolivie) s'est donné comme objectif de restaurer les aspects clinico-nutritionnels et immunologiques lors du traitement d'enfants atteints de malnutrition sévère. Les enfants admis au CRIN sont recrutés parmi ceux qui, âgés de 6 mois à 6 ans, séjournent à l'hôpital materno-infantile. Durant les deux mois de séjour dans le service, ils bénéficient d'un traitement global dispensé par une équipe pluridisciplinaire composée de pédiatres, d'immunologistes, de nutritionnistes, de psychologues et de sociologues. La récupération nutritionnelle est basée sur un modèle diététique en quatre phases. Le suivi de ces enfants au niveau anthropométrique, immunologique (échographie du thymus et sous-populations lymphocytaires) et psychologique est assuré par l'équipe. Les études menées au CRIN ont montré : une atteinte spécifique de l'immunité à médiation cellulaire avec involution thymique et taux élevé de lymphocytes immatures ; un déphasage entre les vitesses de récupération clinico-nutritionnelle et immunologique, qui explique en grande partie les rechutes observées dans la plupart des centres de récupération nutritionnelle ; une possibilité d'accélerer la récupération immunitaire grâce à un supplément journalier en zinc afin qu'elle coïncide avec la récupération nutritionnelle et permette une sortie plus rapide de l'enfant sans risque de rechute. (Résumé d'auteur

    Preliminary results from the STEPHI2009 campaign on the open cluster NGC 1817

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    We present preliminary observational results of the multi-site STEPHI campaign on the cluster NGC 1817. The three observatories involved are San Pedro Martir (Mexico), Xing Long (China) and the Observatorio del Teide (Spain) - giving an ideal combination to maximise the duty cycle. The cluster has 12 known delta Scuti stars and at least two detached eclipsing binary systems. This combination of characteristics is ideal for extracting information about global parameters of the targets, which will in turn impose strict constraints on the stellar models. From an initial comparison with stellar models using the known fundamental parameters, and just the observed pulsation frequencies and measured effective temperatures, it appears that a lower value of initial helium mass fraction will most likely explain the observations of these stars.Comment: 4 pages, proceedings from HELAS IV meeting 2010, Lanzarot

    Software Tool for Acausal Physical Modelling and Simulation

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    Modelling and simulation are key tools for analysis and design of systems and processes from almost any scientific or engineering discipline. Models of complex systems are typically built on acausal Differential-Algebraic Equations (DAE) and discrete events using Object-Oriented Modelling (OOM) languages, and some of their key concepts can be explained as symmetries. To obtain a computer executable version from the original model, several algorithms, based on bipartite symmetric graphs, must be applied for automatic equation generation, removing alias equations, computational causality assignment, equation sorting, discrete-event processing or index reduction. In this paper, an open source tool according to OOM paradigm and developed in MATLAB is introduced. It implements such algorithms adding an educational perspective about how they work, since the step by step results obtained after processing the model equations can be shown. The tool also allows to create models using its own OOM language and to simulate the final executable equation set. It was used by students in a modelling and simulation course of the Automatic Control and Industrial Electronics Engineering degree, showing a significant improvement in their understanding and learning of the abovementioned topics after their assessment

    Escoliosis congénitas causadas por hemivertebras

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    Presentamos un estudio retrospectivo de 26 pacientes diagnosticados de escoliosis congénitas causadas por hemivertebras, liemos analizado la evolución de las curvas según el tipo de hemivértebra, su localización y el tratamiento recibido. Se han obtenido los peores resultados en las niñas, cuando el diagnóstico se realizó después de los 10 años de edad, en las curvas localizadas en la región toracolumbar, en las hemivértebras múltiples y, dentro de ellas, en las unilaterales segmentadas no adyacentes y en los pacientes tratados ortopédicamente.A retrospective study of 26 patients with congenital scoliosis due to hemivertebra was conducted. Curve progression was analysed regarding the type of hemivertebra, its localization, and the applied treatment. The worst results were found in girls, in cases who were diagnosed with more than to years of age, in thoraco-lumbar curves, in multiple hemivertebra, especially in non-adjacent segmented unilateral hemivertebra and, finally, in patients treated with orthopaedic methods

    Multi-site observations of Delta Scuti stars 7 Aql and 8 Aql (a new Delta Scuti variable): The twelfth STEPHI campaign in 2003

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    We present an analysis of the pulsation behaviour of the Delta Scuti stars 7 Aql (HD 174532) and 8 Aql (HD 174589) -- a new variable star -- observed in the framework of STEPHI XII campaign during 2003 June--July. 183 hours of high precision photometry were acquired by using four-channel photometers at three sites on three continents during 21 days. The light curves and amplitude spectra were obtained following a classical scheme of multi-channel photometry. Observations in different filters were also obtained and analyzed. Six and three frequencies have been unambiguously detected above a 99% confidence level in the range 0.090 mHz--0.300 mHz and 0.100 mHz-- 0.145 mHz in 7 Aql and 8 Aql respectively. A comparison of observed and theoretical frequencies shows that 7 Aql and 8 Aql may oscillate with p modes of low radial orders, typical among Delta Scuti stars. In terms of radial oscillations the range of 8 Aql goes from n=1 to n=3 while for 7 Aql the range spans from n=4 to n=7. Non-radial oscillations have to be present in both stars as well. The expected range of excited modes according to a non adiabatic analysis goes from n=1 to n=6 in both stars.Comment: 8 pages, 7 fugures, 5 tables, accepted for publication in Astronomical Journa

    Pulsational frequencies of the eclipsing delta-Scuti star HD 172189

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    The eclipsing delta-Scuti star HD 172189 is a probable member of the open cluster IC 4756 and a promising candidate target for the CoRoT mission. The detection of pulsation modes is the first step in the asteroseismological study of the star. Further, the calculation of the orbital parameters of the binary system allows us to make a dynamical determination of the mass of the star, which works as an important constraint to test and calibrate the asteroseismological models. From a detailed frequency analysis of 210 hours of photometric data of HD 172189 obtained from the STEPHI XIII campaign we have identified six pulsation frequencies with a confidence level of 99% and a seventh with a 65% confidence level in the range between 100-300 uHz. In addiction, three eclipses were observed during the campaign, allowing us to improve the determination of the orbital period of the system.Comment: 6 pages, 7 figure
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