3,804 research outputs found

    Room temperature ferromagnetic-like behavior in Mn-implanted and post-annealed InAs layers deposited by Molecular Beam Epitaxy

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    We report on the magnetic and structural properties of Ar and Mn implanted InAs epitaxial films grown on GaAs (100) by Molecular Beam Epitaxy (MBE) and the effect of Rapid Thermal Annealing (RTA) for 30 seconds at 750C. Channeling Particle Induced X- ray Emission (PIXE) experiments reveal that after Mn implantation almost all Mn atoms are subsbtitutional in the In-site of the InAs lattice, like in a diluted magnetic semiconductor (DMS). All of these samples show diamagnetic behavior. But, after RTA treatment the Mn-InAs films exhibit room-temperature magnetism. According to PIXE measurements the Mn atoms are no longer substitutional. When the same set of experiments were performed with As as implantation ion all of the layers present diamagnetism without exception. This indicates that the appearance of room-temperature ferromagnetic-like behavior in the Mn-InAs-RTA layer is not related to lattice disorder produce during implantation, but to a Mn reaction produced after a short thermal treatment. X-ray diffraction patterns (XRD) and Rutherford Back Scattering (RBS) measurements evidence the segregation of an oxygen deficient-MnO2 phase (nominally MnO1.94) in the Mn-InAs-RTA epitaxial layers which might be on the origin of room temperature ferromagnetic-like response observed.Comment: 16 pages, 5 figures. Acepted in J. Appl. Phy

    X-ray spectral variability of seven LINER nuclei with XMM-Newton and Chandra data

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    One of the most important features in active galactic nuclei (AGN) is the variability of their emission. Variability has been discovered at X-ray, UV, and radio frequencies on time scales from hours to years. Among the AGN family and according to theoretical studies, Low-Ionization Nuclear Emission Line Region (LINER) nuclei would be variable objects on long time scales. Our purpose is to investigate spectral X-ray variability in LINERs and to understand the nature of these kinds of objects, as well as their accretion mechanism. Chandra and XMM-Newton public archives were used to compile X-ray spectra of seven LINER nuclei at different epochs with time scales of years. To search for variability we fit all the spectra from the same object with a set of models, in order to identify the parameters responsible for the variability pattern. We also analyzed the light curves in order to search for short time scale (from hours to days) variability. Whenever possible, UV variability was also studied. We found spectral variability in four objects, with variations mostly related to hard energies (2-10 keV). These variations are due to changes in the soft excess, and/or changes in the absorber, and/or intrinsic variations of the source. Another two galaxies seem not to vary. Short time scale variations during individual observations were not found. Our analysis confirms the previously reported anticorrelation between the X-ray spectral index and the Eddington ratio, and also the correlation between the X-ray to UV flux ratio and the Eddington ratio. These results support an Advection Dominated Accretion Flow (ADAF) as the accretion mechanism in LINERs.Comment: 35 pages, 53 figures, recently accepted pape

    X-ray spectral variability of Seyfert 2 galaxies

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    Variability across the electromagnetic spectrum is a property of AGN that can help constraining the physical properties of these galaxies. This is the third of a serie of papers with the aim of studying the X-ray variability of different families of AGN. The main purpose of this work is to investigate the variability pattern in a sample of optically selected type 2 Seyfert galaxies. We use the 26 Seyferts in the Veron-Cetty and Veron catalogue with data available from Chandra and/or XMM-Newton public archives at different epochs, with timescales ranging from a few hours to years. All the spectra of the same source are simultaneously fitted and we let different parameters to vary in the model. Whenever possible, short-term variations and/or long-term UV flux variations are studied. We divide the sample in Compton-thick, Compton-thin, and changing-look candidates. Short-term variability at X-rays is not found. From the 25 analyzed sources, 11 show long-term variations; eight (out of 11) are Compton-thin, one (out of 12) is Compton-thick, and the two changing-look candidates are also variable. The main driver for the X-ray changes is related to the nuclear power (nine cases), while variations at soft energies or related with absorbers at hard X-rays are less common, and in many cases these variations are accompained with variations of the nuclear continuum. At UV frequencies nuclear variations are nor found. We report for the first time two changing-look candidates, MARK273 and NGC7319. A constant reflection component located far away from the nucleus plus a variable nuclear continuum are able to explain most of our results; the Compton-thick candidates are dominated by reflection, which supresses their continuum making them seem fainter, and not showing variations, while the Compton-thin and changing-look candidates show variations.Comment: Accepted for publication in A&

    X-ray spectral variability of LINERs selected from the Palomar sample

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    Variability is a general property of active galactic nuclei (AGN). At X-rays, the way in which these changes occur is not yet clear. In the particular case of low ionisation nuclear emission line region (LINER) nuclei, variations on months/years timescales have been found for some objects, but the main driver of these changes is still an open question. The main purpose of this work is to investigate the X-ray variability in LINERs, including the main driver of such variations, and to search for eventual differences between type 1 and 2 objects. We use the 18 LINERs in the Palomar sample with data retrieved from Chandra and/or XMM-Newton archives corresponding to observations gathered at different epochs. All the spectra for the same object are simultaneously fitted in order to study long term variations. The nature of the variability patterns are studied allowing different parameters to vary during the spectral fit. Whenever possible, short term variations from the analysis of the light curves and UV variability are studied.Comment: 49 pages, accepted. arXiv admin note: text overlap with arXiv:1305.222

    Comparison of theoretical heat transfer model with results from experimental monitoring installed in a refurbishment with ventilated facade

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    One of the main points to consider when a building is renovated is the improvement of its energy efficiency, minimizing the heat loss through the enclosures and its heating consumption. Under this scope idea a ventilated facade was designed and incorporated in an educational building located in the city of Burgos (Spain). The main objective of this document is a comparison between the theoretical model of heat transfer across the building envelope separating the environment and the interior space, and the heat intake through a linear regression model with installed experimental monitoring. For this it has been necessary to carry out an exhaustive study of the thermal transmission of each one of the materials that make up the thermal envelope of the building, as well as the linear thermal bridges that can be produced before and after the renovation. In addition, thanks to the monitoring installed in the demonstrator building, the interior and exterior temperatures and the heat consumption of each of the radiators is known. In this way expected and real energy savings have been compared

    Diseño de Metodologías Activas para Másteres

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    El objetivo de la Universidad de Burgos desde el Máster en Inspección, Restauración, Rehabilitación y Eficiencia Energética de Edificación (MIREE), es la implementación de metodologías docentes activas con el fin de la formación del alumnado, a través de casos concretos y reales que adicionalmente reportarán un beneficio social. Alguno de estos métodos pueden ser el estudio de casos, la resolución de ejercicios y problemas, el aprendizaje basado en problemas y orientado a proyectos, el aprendizaje cooperativo, etc. Lo que pretendemos con las metodologías activas de aprendizaje es, que los alumnos adquieran las competencias propuestas en el programa docente, desarrollando un aprendizaje profundo en cada una de ellas. Para ello debemos evitar que el profesorado monopolice la docencia, y es necesario comunicarles tanto al alumnado como al profesorado, que la docencia es una inversión en beneficio mutuo. La realización de este tipo de proyectos favorece notablemente a los alumnos ya que desarrollan la motivación de aprendizaje o puesta en práctica de las enseñanzas recibidas, pero lo que sin duda es motivador para ellos es el reconocimiento social al trabajo realizado. Esto se ve reflejado en la Estrategia Europea 2020 a nivel universitario que habla de reforzar la cooperación entre la Universidad, Investigación y Empresa

    Analysis of Documental Heritage of CETA in Standardization of the Spanish Manufacturing Automotive Industry

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    AbstractStandardization has taken an active role in the development of several main industrial sectors and the automotive sector has been one of them. Current work shows the collection, analysis, revision and management process developed on CETA (Center of Automotive Technical Study) standards related to the manufacturing automotive sector, an unknown element of Spanish standardization heritage. Also, a comparative evaluation between CETA standards and current UNE standards has been performed. The results show that CETA standards have had a positive influence in the evolution of the automotive sector as well as an important contribution to the contents of the UNE standards

    Scattering of surface plasmon polaritons by one-dimensional inhomogeneities

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    The scattering of surface plasmons polaritons by a one-dimensional defect of the surface is theoretically studied, by means of both Rayleigh and modal expansions. The considered defects are either relief perturbations or variations in the permittivity of the metal. The dependence of transmission, reflection and out-of-plane scattering on parameters defining the defect is presented. We find that the radiated energy is forwardly directed (with respect to the surface plasmon propagation) in the case of an impedance defect. However, for relief defects, the radiated energy may be directed into backward or forward (or both) directions, depending on the defect width.Comment: 10 pages, 5 figures, corrected typos, some minor modifications in figures. Accepted in Phys. Rev.

    Methodological issues in the measurement of alcohol consumption: The importance of drinking patterns

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    Medir correctamente el consumo de alcohol es fundamental para investigar de forma fiable sus efectos en salud. Sin embargo, ésta estimación resulta enormemente compleja, tanto por la diversidad de formas de consumo de alcohol existente como por la gran heterogeneidad en su clasificación. Además, cada patrón de consumo de alcohol puede asociarse a efectos muy diferente sobre la salud, por lo que no tenerlos en consideración cuando estimamos la ingesta de alcohol puede ocultar o confundir su importancia en estos efectos. Todo ello dificulta las comparaciones entre estudios y el establecimiento de asociaciones consistentes que permitan comprender los verdaderos efectos del consumo de alcohol, tanto globales como específicos de cada patrón de bebida. Este trabajo revisa los principales métodos y fuentes de información disponibles en España para estimar los aspectos más relevantes del consumo de alcohol, así como las dificultades y problemas metodológicos más frecuentes en la medición y clasificación de cada uno de estos indicadoresMeasurement of alcohol consumption is essential for proper investigation of its effects on health. However, its estimation is extremely complex, because of the diversity of forms of alcohol consumption and their highly heterogeneous classification. Moreover, each form may have different effects on health; therefore, not considering the most important drinking patterns when estimating alcohol in take could mask the important role of consumption patterns in these effects. All these issues make it very difficult to compare the results of different studies and to establish consistent associations for understanding the true effects of alcohol consumption, both overall and specific to each drinking pattern. This article reviews the main methods and sources of information available in Spain for estimating the most important aspects of alcohol consumption, as well as the most frequent methodological problems encountered in the measurement and classification of drinking patterns.Este estudio se realizó en el marco del Grupo de Trabajo sobre Alcohol de la Sociedad Española de Epidemiología con la ayuda económica del Plan Nacional sobre Drogas que ha contribuido a su funcionamiento (órdenes SSI 2800/2012 y 131/2013
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