72 resultados para galaxy : quasar : individual
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Este estudio evalúa la eficacia de la Psicoterapia Psicoanalítica Focal y Breve (PPFB) en 46 mujeres maltratadas por su pareja atendidas en la Unitat d’Atenció Especialitzada per a Dones Maltractades (UNADOM) de la Fundació Vidal i Barraquer de Barcelona, a través del Millon Clinical Multiaxial Inventory-II (MCMI-II). La UNADOM es un servicio de asistencia público y gratuito subvencionado por la Generalitat de Catalunya destinado a mujeres maltratadas que necesitan atención psicológica en régimen ambulatorio. Se tuvieron en cuenta los resultados obtenidos en el MCMI-II en la fase inicial de evaluación y una vez finalizado el tratamiento. Los resultados revelan que al inicio de la terapia las tres escalas básicas de personalidad que obtuvieron la media más elevada fueron la Dependiente, la Autodestructiva y la Fóbica. En cambio, una vez finalizada la terapia individual, estas mismas escalas presentaban puntuaciones medias inferiores y estadísticamente significativas. Tan sólo la escala Compulsiva mostraba puntuaciones superiores al punto de corte TB>75. Se discuten los resultados obtenidos y se insta a que futuros trabajos proporcionen mayor evidencia empírica de las complejas interacciones que se producen entre los dos miembros de la pareja en situaciones de maltrato para poder diseñar estrategias de prevención y de tratamientos eficaces y realistas.
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Background: Recent research based on comparisons between bilinguals and monolinguals postulates that bilingualism enhances cognitive control functions, because the parallel activation of languages necessitates control of interference. In a novel approach we investigated two groups of bilinguals, distinguished by their susceptibility to cross-language interference, asking whether bilinguals with strong language control abilities ('non-switchers") have an advantage in executive functions (inhibition of irrelevant information, problem solving, planning efficiency, generative fluency and self-monitoring) compared to those bilinguals showing weaker language control abilities ('switchers"). Methods: 29 late bilinguals (21 women) were evaluated using various cognitive control neuropsychological tests [e.g., Tower of Hanoi, Ruff Figural Fluency Task, Divided Attention, Go/noGo] tapping executive functions as well as four subtests of the Wechsler Adult Intelligence Scale. The analysis involved t-tests (two independent samples). Non-switchers (n = 16) were distinguished from switchers (n = 13) by their performance observed in a bilingual picture-naming task. Results: The non-switcher group demonstrated a better performance on the Tower of Hanoi and Ruff Figural Fluency task, faster reaction time in a Go/noGo and Divided Attention task, and produced significantly fewer errors in the Tower of Hanoi, Go/noGo, and Divided Attention tasks when compared to the switchers. Non-switchers performed significantly better on two verbal subtests of the Wechsler Adult Intelligence Scale (Information and Similarity), but not on the Performance subtests (Picture Completion, Block Design). Conclusions: The present results suggest that bilinguals with stronger language control have indeed a cognitive advantage in the administered tests involving executive functions, in particular inhibition, self-monitoring, problem solving, and generative fluency, and in two of the intelligence tests. What remains unclear is the direction of the relationship between executive functions and language control abilities.
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A simple chaotic flow is presented, which when driven by an identical copy of itself, for certain initial conditions, is able to display generalized synchronization instead of identical synchronization. Being that the drive and the response are observed in exactly the same coordinate system, generalized synchronization is demonstrated by means of the auxiliary system approach and by the conditional Lyapunov spectrum. This is interpreted in terms of changes in the structure of the system stationary points, caused by the coupling, which modify its global behavior.
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Postprint (published version)
Resumo:
INDISIM-YEAST, an individual-based simulator, models the evolution of a yeast population by settingup rules of behaviour for each individual cell according to their own biological rules and characteristics. Ittakes into account the uptake, metabolism, budding reproduction and viability of the yeast cells, over aperiod of time in the bulk of a liquid medium, occupying a three dimensional closed spatial grid with twokinds of particles (glucose and ethanol). Each microorganism is characterized by its biomass, genealogicalage, states in the budding cellular reproduction cycle and position in the space among others. Simulationsare carried out for population properties (global properties), as well as for those properties that pertain toindividual yeast cells (microscopic properties). The results of the simulations are in good qualitativeagreement with established experimental trends.
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Context. The understanding of Galaxy evolution can be facilitated by the use of population synthesis models, which allow to test hypotheses on the star formation history, star evolution, as well as chemical and dynamical evolution of the Galaxy. Aims. The new version of the Besanc¸on Galaxy Model (hereafter BGM) aims to provide a more flexible and powerful tool to investigate the Initial Mass Function (IMF) and Star Formation Rate (SFR) of the Galactic disc. Methods. We present a new strategy for the generation of thin disc stars which assumes the IMF, SFR and evolutionary tracks as free parameters. We have updated most of the ingredients for the star count production and, for the first time, binary stars are generated in a consistent way. We keep in this new scheme the local dynamical self-consistency as in Bienayme et al (1987). We then compare simulations from the new model with Tycho-2 data and the local luminosity function, as a first test to verify and constrain the new ingredients. The effects of changing thirteen different ingredients of the model are systematically studied. Results. For the first time, a full sky comparison is performed between BGM and data. This strategy allows to constrain the IMF slope at high masses which is found to be close to 3.0, excluding a shallower slope such as Salpeter"s one. The SFR is found decreasing whatever IMF is assumed. The model is compatible with a local dark matter density of 0.011 M pc−3 implying that there is no compelling evidence for significant amount of dark matter in the disc. While the model is fitted to Tycho2 data, a magnitude limited sample with V<11, we check that it is still consistent with fainter stars. Conclusions. The new model constitutes a new basis for further comparisons with large scale surveys and is being prepared to become a powerful tool for the analysis of the Gaia mission data.
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Objetivos. Valorar la utilidad de un fórum virtual sobre la discusión de un caso clínico por grupos para la presentación de un trabajo individual. Material y métodos. En uno de los seminarios de la asignatura Enfermedades del Aparato Respiratorio y ORL del grado de Medicina, se creó un fórum virtual para discutir un caso clínico por grupos, antes de presentar un trabajo individual. Se realizaron cuatro grupos (A, B, C y D) y se abrieron cuatro temas. Cada grupo sólo podía participar en uno, pero tenían que observar la evolución de los otros foros. El trabajo individual consistía en contestar a varias preguntas planteadas por el profesor relacionadas con el desarrollo del caso clínico virtual. Para analizar los resultados de la experiencia se valoró: el número de participaciones en el foro, el número de participaciones por grupo, la nota del trabajo individual y la opinión del profesor Resultados. Se realizaron 129 participaciones al foro. El grupo A fue el que más participó (27%). El 78% de los alumnos obtuvo una nota comprendida entre el 7 y el 9. Del análisis cualitativo del trabajo individual se observó que los alumnos contestaban correctamente las preguntas, pero no se basaban en lo que sus compañeros habían desarrollado en el foro. Conclusiones. Los foros virtuales basados en la discusión de casos clínicos pueden facilitar el aprendizaje colaborativo en alumnos del grado de Medicina.
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La constitució d'una societat de capital pot constituir un excel·lent instrument per facilitar la transició intergeneracional en aquelles empreses el titular dels quals és una persona física i els descendents han pres la decisió d'entrada a temps complet en l'organització empresarial. En aquest sentit, el trànsit de la condició d'empresari individual a empresari social no només permet la conservació de l'empresa més enllà de la vida del seu actual titular simplificant el procés hereditari sinó que permet gaudir, entre d'altres, dels avantatges de la limitació de responsabilitat per deutes i de la separació del patrimoni civil dels socis del patrimoni necessari per l'exercici de l'empresa reduint així els riscos econòmics patrimonials. Addicionalment, la relativa flexibilitat del règim jurídic de les societats de capital permet que els socis tinguin la possibilitat d'adequar-lo a les seves específiques necessitats i conveniències.
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La constitución de una sociedad de capital puede constituir un exelente instrumento para facilitar la transición intergeneracional en aquellas empresas en la que su titular es una persona fisica y sus descendientes han tomado la decisión de entrada a tiempo completo en la organización empresarial. En este sentido, el tránsito de la condición de empresario individual a empresario social no solo permite la conservación de la empresa más allá de la vida de su titular actual, simplificando el proceso hereditario, sino que además permite disfrutar de las ventajas de la limitación de la responsabilidad por deudas y de la separación del patrimonio civil de los socios del patrimonio necesario para el ejercicio de la empresa, reduciendo así los riesgos económicos patrimoniales. Adicionalmente, la relativa flexibilidad del régimen jurídico de las sociedades de capital permite que los socios tengan la posibilidad de adecuarlo a sus necesidades específicas.
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The accretion of matter onto a massive black hole is believed to feed the relativistic plasma jets found in many active galactic nuclei (AGN). Although some AGN accelerate particles to energies exceeding 1012 electron volts and are bright sources of very-high-energy (VHE) γ-ray emission, it is not yet known where the VHE emission originates. Here we report on radio and VHE observations of the radio galaxy Messier 87, revealing a period of extremely strong VHE γ-ray flares accompanied by a strong increase of the radio flux from its nucleus. These results imply that charged particles are accelerated to very high energies in the immediate vicinity of the black hole.
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Context. The understanding of Galaxy evolution can be facilitated by the use of population synthesis models, which allow to test hypotheses on the star formation history, star evolution, as well as chemical and dynamical evolution of the Galaxy. Aims. The new version of the Besanc¸on Galaxy Model (hereafter BGM) aims to provide a more flexible and powerful tool to investigate the Initial Mass Function (IMF) and Star Formation Rate (SFR) of the Galactic disc. Methods. We present a new strategy for the generation of thin disc stars which assumes the IMF, SFR and evolutionary tracks as free parameters. We have updated most of the ingredients for the star count production and, for the first time, binary stars are generated in a consistent way. We keep in this new scheme the local dynamical self-consistency as in Bienayme et al (1987). We then compare simulations from the new model with Tycho-2 data and the local luminosity function, as a first test to verify and constrain the new ingredients. The effects of changing thirteen different ingredients of the model are systematically studied. Results. For the first time, a full sky comparison is performed between BGM and data. This strategy allows to constrain the IMF slope at high masses which is found to be close to 3.0, excluding a shallower slope such as Salpeter"s one. The SFR is found decreasing whatever IMF is assumed. The model is compatible with a local dark matter density of 0.011 M pc−3 implying that there is no compelling evidence for significant amount of dark matter in the disc. While the model is fitted to Tycho2 data, a magnitude limited sample with V<11, we check that it is still consistent with fainter stars. Conclusions. The new model constitutes a new basis for further comparisons with large scale surveys and is being prepared to become a powerful tool for the analysis of the Gaia mission data.