Hegel y su perfil psicopatológico, a la luz de su concepción filosófica de la religión.

El presente estudio lleva a cabo una valoración crítica del pensamiento hegeliano, a la luz de los resortes psíquicos que explican su posición filosófica en materia de religión. En particular se aborda la transposición que hace de Dios a su persona al hablar en términos racionales de autoconciencia, dada la peculiar teología de la historia que propone. Se hace una presentación crítica basada en algunos de los detractores cercanos a esta visión, para encontrar una interpretación que nos permita ver una tipología más cercana a sus patologías mentales, utilizando para ello el método de aproximaciones sucesivas. Para este fin, se utilizan teorías psiquiátricas diversas que comprenden bien este fenómeno desde sus particulares semiologías y análisis caracterológicos

El Dios Geométrico de Baruch Spinoza

This paper presents the metaphysical theory of Baruch Spinoza’s geometrical God as laid out in his Ethica, Ordine Geometrico Demonstrata of 1677. We will split this study into four sections, i.e. God, the Soul, Knowledge, and Physics, although all the parts of the Ethics relate directly to God, since he constitutes their ultimate basis. In our opinion, Spinoza´s Ethics constitute the highest form of rationalistic monism in modernity, as we will attempt to show in the following pages.El presente artículo es una síntesis de la doctrina del Dios geométrico de Baruch Spinoza, contenida en su Ethica, Ordine Geometrico Demonstrata de 1677. Dividiremos el estudio en cuatro secciones, a saber, de Dios, del Alma, del Conocimiento y de la Física, aunque, en definitiva, todas las partes de la Ética tienen relación directa con Dios, pues en él hallan su último fundamento. A nuestro juicio, la Ética spinoziana es la expresión más lograda del monismo racionalista de la modernidad, como intentaremos mostrar en las páginas siguientes. &nbsp

¿A quiénes afecta el desempleo? análisis de la tasa de incidencia en Colombia

El análisis de la dimensión de riesgo en el estudio del desempleo, complementa el estudio de aspectos como su tipología, la importancia de la intermediación laboral o la vulnerabilidad de ciertos grupos. En este sentido, la tasa de incidencia representa un indicador compuesto que tiene en cuenta el volumen de desempleados y la persistencia en este estado mediante la incorporación de la duración media del desempleo. El análisis de la tasa de incidencia permite caracterizar de manera más completa a quienes tienen una mayor probabilidad de entrar en el desempleo o permanecer en esta situación. . Se encuentra que en Colombia existen diferencias significativas entre la tasa de desempleo y la tasa de incidencia, lo que implica que la situación del mercado de trabajo no sólo se explica por el efecto que los choques económicos tienen sobre la composición de la oferta y demanda de trabajo sino también por los fenómenos de duración en los diferentes estados laborales. Estos eventos se pueden considerar igualmente importantes para explicar la dinámica de corto y mediano plazo del mercado laboral.****The analysis of the risk dimension of unemployment adds on the study of issues such as its typology (frictional, structural and cyclical), active-search methods and vulnerability to unemployment. On this sense, the incidence rate of unemployment is a composed indicator which combines both the level of unemployment and the persistence of it (its duration). An analytical decomposition of the different features of unemployment incidence allows for a deeper characterization of vulnerability to the likelihood of becoming unemployed and to remain in such state. We find that in the Colombian labour market there are significant differences between the unemployment rate and the incidence rate, which implies that the outcomes of the labour market are not just explained by the effect of aggregate shocks but by the duration effects of the different labour states, which are also important on explaining the short and long run dynamics of the labour market.Tasa de desempleo, búsqueda de empleo, persistencia del desempleo, incidenciadel desempleo

Crossing the phantom divide in an interacting generalized Chaplygin gas

Unified generalized Chaplygin gas models assuming an interaction between dark energy and dark matter fluids have been previously proposed. Following these ideas, we consider a particular relation between dark densities, which allows the possibility of a time varying equation of state for dark energy that crosses the phantom divide at a recent epoch. Moreover, these densities decay during all the evolution of the Universe, avoiding a Big Rip. We find also a scaling solution, i.e. these densities are asymptotically proportional in the future, which contributes to the solution of the coincidence problem.Comment: Improved version, 10 pages, 4 figures, References adde

Identification by means of molecular tools of the microbiota responsible for the formation of histamine accumulated in commercial cheeses in Spain

Histamine intoxication is an important food safety and public health concern. Ripened cheeses are the most common dairy products in which histamine can accumulate. Histamine is formed by the microbiota present in cheese by decarboxylation of histidine, due to the action of the histidine decarboxylase. This study's objective was to identify the responsible for the formation of histamine accumulated in commercial cheeses. The content of histamine of 39 different types of cheeses marketed in Spain, of varying milk origin, was assessed. About one third of the cheeses analysed contained more than 200 mg/kg histamine; two cheeses exceeded 500 mg/kg histamine, the consumption of such cheeses can be harmful or even toxic for consumers. The five cheeses with the highest histamine concentrations were selected for in-depth molecular analysis. Firstly, bacterial and yeast isolates were obtained, and then the total genetic material from the cheeses was analysed, in order to verify the putative presence of the hdc histidine decarboxylase gene. In order to identify the histamine producing microorganisms, the nucleotide sequences of the histidine decarboxylase genes from the cheeses were amplified, and subjected them to Sanger sequencing. In four of the five selected cheeses, the main histamine producer was identified as Lentilactobacillus parabuchneri, whereas in the remaining cheese it was Tetragenococcus halophilus. The hdc gene was located in an unstable plasmid, only present in that cheese sample. Since all histamine producing microorganisms identified in this study are not part of the species used in cheese starter cultures, an improvement of hygienic manufacturing practices and/or thermal treatments for microbial inactivation in milk may be considered to prevent histamine accumulation in cheeses during ripening

Calibración de Microscopios Confocales

El microscopio confocal ha sido durante mucho tiempo un instrumento de observación tridimensional con múltiples aplicaciones especialmente dentro de la biología. Sin embargo en los últimos años ha comenzado a ser utilizado como instrumento de medida en diferentes áreas de la ingeniería. En la actualidad existen muchas especificaciones de productos (dimensionales, angulares, acabado superficial) en las escalas micrométricas y nanométricas que pueden o podrían ser verificadas utilizando este instrumento. Pero para que esta verificación sea válida dentro de un sistema de calidad el microscopio confocal debe ser trazable. Esta ponencia presenta una solución sencilla a este problema implementada en el Centro Láser de la Universidad Politécnica de Madrid (UPM) que ha permitido dotar de trazabilidad a las medidas dimensionales realizadas en el plano XY y en el eje Z de su microscopio confocal. The confocal microscope has been a three-dimensional observation instrument with multiple applications especially in biology. However in recent years has begun to be used as a measuring instrument contact in various engineering fields. At present there are many product specifications (size, angular, surface roughness) in the micrometer and nano scales that can or could be verified using this instrument. But this verification is only valid within a quality system if the confocal microscope is traceable. This paper presents a simple solution to this problem implemented in the Laser Centre of the Polytechnic University of Madrid (UPM). This solution provides traceablity to the size measurements made in the XY plane and the Z-axis

High resolution spectroscopy of the high velocity hot post-AGB star LS III +52 24 (IRAS 22023+5249)

The first high-resolution (R~50,000) optical spectrum of the B-type star, LS III +52 24, identified as the optical counterpart of the hot post-AGB candidate IRAS 22023+5249 (I22023) is presented. We report the detailed identifications of the observed absorption and emission features in the full wavelength range (4290-9015 A) as well as the atmospheric parameters and photospheric abundances (under the Local Thermodinamic Equilibrium approximation) for the first time. The nebular parameters (Te, Ne) are also derived. We estimate Teff=24,000 K, log g=3.0, xi=7 kms-1 and the derived abundances indicate a slightly metal-deficient evolved star with C/O<1. The observed P-Cygni profiles of hydrogen and helium clearly indicate on-going post-AGB mass loss. The presence of [N II] and [S II] lines and the non-detection of [O III] indicate that photoionisation has just started. The observed spectral features, large heliocentric radial velocity, atmospheric parameters, and chemical composition indicate that I22023 is an evolved post-AGB star belonging to the old disk population. The derived nebular parameters (Te=7000 K, Ne=1.2x104 cm-3) also suggest that I22023 may be evolving into a compact, young low-excitation Planetary Nebula. Our optical spectroscopic analysis together with the recent Spitzer detection of double-dust chemistry (the simultaneous presence of carbonaceous molecules and amorphous silicates) in I22023 and other B-type post-AGB candidates may point to a binary system with a dusty disk as the stellar origin common to the hot post-AGB stars with O-rich central stars.Comment: Accepted for publication in MNRAS (22 pages, 4 figures, and 8 tables). arXiv admin note: substantial text overlap with arXiv:0707.059

Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations

We present the study of nineteen low X-ray luminosity galaxy clusters (L$_X \sim$ 0.5--45 $\times$ $10^{43}$ erg s$^{-1}$), selected from the ROSAT Position Sensitive Proportional Counters (PSPC) Pointed Observations (Vikhlinin et al. 1998) and the revised version of Mullis et al. (2003) in the redshift range of 0.16 to 0.7. This is the introductory paper of a series presenting the sample selection, photometric and spectroscopic observations and data reduction. Photometric data in different passbands were taken for eight galaxy clusters at Las Campanas Observatory; three clusters at Cerro Tololo Interamerican Observatory; and eight clusters at the Gemini Observatory. Spectroscopic data were collected for only four galaxy clusters using Gemini telescopes. With the photometry, the galaxies were defined based on the star-galaxy separation taking into account photometric parameters. For each galaxy cluster, the catalogues contain the PSF and aperture magnitudes of galaxies within the 90\% completeness limit. They are used together with structural parameters to study the galaxy morphology and to estimate photometric redshifts. With the spectroscopy, the derived galaxy velocity dispersion of our clusters ranged from 507 km~s$^{-1}$ for [VMF98]022 to 775 km~s$^{-1}$ for [VMF98]097 with signs of substructure. Cluster membership has been extensively discussed taking into account spectroscopic and photometric redshift estimates. In this sense, members are the galaxies within a projected radius of 0.75 Mpc from the X-ray mission peak and with cluster centric velocities smaller than the cluster velocity dispersion or 6000 km~s$^{-1}$, respectively. These results will be used in forthcoming papers to study, among the main topics, the red cluster sequence, blue cloud and green populations; the galaxy luminosity function and cluster dynamics.Comment: 13 pages, 6 tables, 9 figures. Uses emulateapj. Accepted for publication in The Astronomical Journal. Some formatting errors fixe

Valoración aristotélico-argumentativa del caso Iguala, a propósito de la Comisión por la Verdad y la Justicia

El propósito de esta reflexión es la de analizar el contenido del derecho humano a la creación artística de los individuos per se, independientemente de que su obra pueda enmarcarse dentro de las manifestaciones culturales propias o características de una determinada identidad colectiva. Igualmente, el trabajo trata de responder a la cuestión acerca de si las condiciones materiales de los artistas deben verse satisfechas por el mercado o si es predicable algún tipo de deber por parte de los poderes públicos que garanticen la existencia de creadores artísticos libres y con ello la emancipación del individuo y el carácter plural y democrático de una sociedad