High mass microquasars and low latitude gamma-ray sources

Population studies of unidentified EGRET sources suggest that there exist at least three different populations of galactic gamma-ray sources. One of these populations is formed by young objects distributed along the galactic plane with a strong concentration toward the inner spiral arms of the Galaxy. Variability, spectral and correlation analysis indicate that this population is not homogeneous. In particular, there is a subgroup of sources that display clear variability in their gamma-ray fluxes on timescales from days to months. Following the proposal by Kaufman Bernad\'o et al. (2002), we suggest that this group of sources might be high-mass microquasars, i.e. accreting black holes or neutron stars with relativistic jets and early-type stellar companions. We present detailed inhomogeneous models for the gamma-ray emission of these systems that include both external and synchrotron self-Compton interactions. We have included effects of interactions between the jet and all external photon fields to which it is exposed: companion star, accretion disk, and hot corona. We make broadband calculations to predict the spectral energy distribution of these objects from radio up to GeV energies. The results and predictions can be tested by present and future gamma-ray instruments like INTEGRAL, AGILE, and GLAST.

AGNs and microquasars as high-energy gamma-ray sources

The possible associations between the microquasars LS 5039 and LS I +61 303 and the EGRET sources 3EG J1824-1514 and 3EG J0241+6103 suggest that microquasars could also be sources of high-energy gamma-rays. In this work, we present a detailed numerical inverse Compton (IC) model, based on a microquasar scenario, that reproduces the high-energy gamma-ray spectra and variability observed by EGRET for the mentioned sources. Our model considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet that interact through IC scattering with both the radiation and the magnetic fields.

Poétique des objets chez Sophocle : fonctions dramatiques et valeurs symboliques

La thèse propose une analyse du rôle des objets dans quatre tragédies (Ajax, Trachiniennes, Electre, Philoctèté) et un drame satyrique (Limiers) de Sophocle. Le propos est d'étayer le constat selon lequel les objets ont un rôle prépondérant dans l'économie générale de chacune de ces intrigues et de dégager ce rôle chez cet auteur. L'introduction met en évidence l'émergence du material turn en sciences humaines jusque dans les sciences de l'Antiquité en passant par la littérature et l'anthropologie, souligne le caractère souple et opératoire de la catégorie de l'objet, le lien avec la question du signe et du langage non verbal et relève l'absence d'équivalent en grec ancien pour cette catégorie, avec le problème épistémologique que cela implique pour la présente recherche. L'objet n'est pas abordé ici comme accessoire, mais comme entité participant d'une fiction théâtrale. On distingue les moments où les objets sont susceptibles d'apparaître sur scène des moments où ils apparaissent dans des récits ou des évocations. Dans le monde fictionnel constitué par chaque intrigue, sont envisagés les modes d'apparition textuels et poétiques d'objets intra-fictionnels, dans le cadre du genre théâtral, qui combine discours et actions, avec les décalages et les phénomène de dissimulation et d'ostentation que cela implique. Les métaphores et les images jouent ici un rôle prépondérant. Des analyses circonstanciées en 5 chapitres thématisant les objets et leurs fonctions. Dans I'Ajax, les valeurs liées aux armes, en particulier l'épée d'Hector et le bouclier d'Eurysacès, telles qu'elles apparaissent dans l'épopée, sont transposées dans une logique tragique où le prestige lié à ces armes devient polémique et problématique. Le vêtement sacrificiel des Trachiniennes, auquel répond la figure d'Iole, un personnage largement réifiés, thématise le déséquilibre qui caractérise les relations entre Héraclès et Déjanire, dans le cadre des institutions du mariage et du sacrifice, où s'immisce une dimension sauvage et sournoise. Dans l'Electre, au contexte funéraire et d'appel à la vengeance, auquel renvoie une multitude d'objets (sceptre, hache, lit et autres pièces de mobilier, offrandes, etc.) se superpose une dimension méta-fictionnelle et méta-théâtrale investie par l'urne vide. L'arc du Philoctèté constitue l'enjeu dramatique principal de la tragédie et cristallise un débat polémique de valeurs humaines instables auquel s'oppose une logique divine et collective attachée au passé de l'objet, qui se trouve réorienté vers un avenir glorieux. Un passage par le seul drame satyrique conservé de Sophocle permet de constater que l'objet, une tortue-lyre, possède des caractéristiques similaires transposées dans le contexte satyrique, où l'hybridité, les marqueurs de la civilisation, les attributions des Satyres, mais aussi des traits comiques, jouent un rôle prépondérant. La conclusion tente une synthèse et identifie plusieurs observations transversales : jeux sur la présence et l'absence, décalages entre discours et actions, entre langage verbal et non verbal, modalités d'allusion à des personnages, temporalités et espaces absents, détournement des fonctions d'usage, modalités du don, de l'échange et de la privation, procédures de personnification et de réification, rôle prépondérant dans les modalités de l'accomplissement du destin. A la faveur de l'identification de ces caractéristiques transversales, on tente d'ouvrir le propos sur la question du cadavre, dont le statut semble intermédiaire entre personnage et objet, notamment aussi dans \'Antigone, et la figure d'Oedipe, qui apparaît comme un héros- objet dans les deux tragédies que lui consacre Sophocle, l'Oedipe-roi, et \'Oedipe à Colone.

Innovar, renovar, avaluar

[eng] The new educational context in which we are involved and the facilities of the TIC (Communication Information Technologies) have led to the necessary modification of didactic approach that during years has been used for Pharmaceutical Technology teaching. However, changes/updating and innovation require a simultaneous reflection in order to avoid excessive dispersion of the approach and to channel adequately the pedagogic and didactic effort. On the other hand, it is necessary to evaluate the above initiatives to determinate if these one are on the right track. The Pharmaceutical Technology Teaching Innovation Group of the University of Barcelona has been formed and consolidated in this point of view. In this work, a review of studies carried on by the group, in the exposed purposes, from the beginning of their activities is presented. [spa] El nuevo contexto docente en el que estamos inmersos así como las posibilidades de las TIC (Tecnologías de la Información y de la Comunicación) han conllevado la necesaria modificación de los planteamientos didácticos que durante años han servido de base para las enseñanzas de la Tecnología Farmacéutica. Sin embargo, la renovación/actualización e innovación precisan de una simultánea reflexión a fin de evitar una excesiva dispersión del enfoque y para encauzar adecuadamente el esfuerzo pedagógico y didáctico. Por otra parte, es necesario evaluar dichas iniciativas para determinar si están bien encaminadas. El Grupo de Innovación Docente de Tecnología Farmacéutica de la Universidad de Barcelona se ha creado y consolidado desde esta óptica. En este trabajo se presentan un conjunto de estudios que el grupo ha llevado a cabo, con los fines expuestos, desde el comienzo de sus actividades.

Los nummulítidos (Nummulites y Assilina) del Paleoceno Superior-Eoceno Inferior de la cuenca pirenaica: Sistemaáica.

Se ha realizado el estudio sistemático de los nummulítidos pertenecientes a los géneros Nummulites y Assilina del intervalo Paleoceno Superior - Eoceno Inferior de la Cuenca Pirenaica, a partir de muestras procedentes principalmente del sector meridional de la cuenca. Los taxones descritos se han comparado con especímenes procedentes de otras cuencas de la Mesogea: Alpes suizos (Schlieren- y Gumigelflysch) y austríacos (unidades alóctonas helvéticas), norte de Italia (Verona y Vicenza), plataformas marinas adriáticas (Eslovenia y Croacia), península de Crimea (Ucrania), Cuenca de Haymana (Anatolia central, Turquía), y Salt Range (Pakistán). Se han descrito 98 taxones de nummuiítidos -entre especies y subespecies-, de los cuales: - 66 taxones del género Nummulites, pertenecientes a los grupos de N. perforatus, N. partschi, N. rotularius, N. minewensis, N. globulus, N. laevigatus, N. distans, N. heberti y N. spirectypus. - 32 taxones del género Assilina, pertenecientes a los gmpos de A. spira, A. exponens, A. subgranulosa, A. ammonea, A. canalijera y A. alpina. En este trabajo -y siguiendo las consideraciones de Loeblich y Tappan (1987)- Assilina integra las denominaciones gen6ricas tradicionales de Assilina y Operculina.

Bosque y turismo

This paper presents a number of considerations on the recreational/tourism function offorests and some regulations that should be present in the planning of the public use of forestspace. We are going to examine studies on frequency of use, the features that condition theuse of forests and the criteria that should be present on planning of recreational use of forests

European Study Programme for Advanced Networking Technologies

In this article authors present main objectives and progress of the EU ERASMUS CD project: European Study Programme for Advanced Networking Technologies (ESPANT)

The impact of inbound demand on price levels in tourism municipalities : Empirical evidence from Catalonia

It is usually argued that tourism exerts negative economic impacts in host jurisdictions through the increase in prices linked to increasing demand for basic services and goods from tourists. This paper surveys 149 products in 45 tourism and non-tourism jurisdictions in Catalonia (which represent a total of 18,500 prices) in order to test empirically several hypotheses related to differences in price levels in tourism and non-tourism jurisdictions. The main results show that prices in tourism jurisdictions are not significantly higher than those in non-tourism ones. The analysis suggests that tourists are likely to pay higher prices than natives for some products

Los procesos constructivos de la arquitectura clásica. De la proyección a la ejecución. El caso del Concilium Provinciae Hispaniae Citeriosi de Tarraco

Toda obra arquitectónica necesita de una proyección previa que implique la definición y justificación de sus formas y proporciones, proyección que, a menudo, viene modificada por la realidad ya existente o, en casos de periodos constructivos largos por cambios de opinión, de finalidad o, incluso de promotor. Es el caso del Concilium Provinciae Hispaniae Citerioris de Tarraco, un gran complejo monumental de más de 12 hectáreas de extensión, que necesitó un periodo de tiempo de construcción de entre 70 a 75 años. Los restos arqueológicos conservados permiten la identificación de dos proyectos arquitectónicos sobrepuestos que implican un profundo cambio de proyecto durante el proceso constructivo.

Identifying variable gamma-ray sources through radio observations

We present preliminary results of a campaign undertaken with different radio interferometers to observe a sample of the most variable unidentified EGRET sources. We expect to detect which of the possible counterparts of the gamma-ray sources (any of the radio emitters in the field) varies in time with similar timescales as the gamma-ray variation. If the gamma-rays are produced in a jet-like source, as we have modelled theoretically, synchrotron emission is also expected at radio wavelengths. Such radio emission should appear variable in time and correlated with the gamma-ray variability.

Microquasar models for 3EG J1828+0142 and 3EG J1735-1500

Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies show that variable EGRET sources at low galactic latitudes could be associated with the inner spiral arms. The variable nature and the location in the Galaxy of the high-mass microquasars, concentrated in the galactic plane and within 55 degrees from the galactic center, give to these objects the status of likely counterparts of the variable low-latitude EGRET sources. We consider in this work the two most variable EGRET sources at low-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar model to explain the EGRET data in consistency with the observations at lower energies (from radio frequencies to soft gamma-rays) within the EGRET error box.

The octagon, the hendecagon and the approximation of pi: the geometric design of the clypeus in the enclosure of Imperial cult in Tarraco

The ancient temple dedicated to the Roman Emperor Augustus on the hilltop of Tarraco (today’s Tarragona), was the main element of the sacred precinct of the Imperial cult. It was a two hectare square, bordered by a portico with an attic decorated with a sequence of clypeus (i.e. monumental shields) made with marble plates from the Luni-Carrara’s quarries. This contribution presents the results of the analysis of a three-dimensional photogrammetric survey of one of these clipeus, partially restored and exhibited at the National Archaeological Museum of Tarragona. The perimeter ring was bounded by a sequence of meanders inscribed in a polygon of 11 sides, a hendecagon. Moreover, a closer geometric analysis suggests that the relationship between the outer meander rim and the oval pearl ring that delimited the divinity of Jupiter Ammon can be accurately determined by the diagonals of an octagon inscribed in the perimeter of the clypeus. This double evidence suggests a combined layout, in the same design, of an octagon and a hendecagon. Hypothetically, this could be achieved by combining the octagon with the approximation to Pi used in antiquity: 22/7 of the circle’s diameter. This method allows the drawing of a hendecagon with a clearly higher precision than with other ancient methods. Even the modelling of the motifs that separate the different decorative stripes corroborates the geometric scheme that we propose.

Radio continuum and near-infrared study of the MGRO J2019+37 region

MGRO J2019+37 is an unidentified extended source of very high energy gamma-rays originally reported by the Milagro Collaboration as the brightest TeV source in the Cygnus region. Its extended emission could be powered by either a single or several sources. The GeV pulsar AGL J2020.5+3653 , discovered by AGILE and associated with PSR J2021+3651 , could contribute to the emission from MGRO J2019+37 . Aims. Our aim is to identify radio and near-infrared sources in the field of the extended TeV source MGRO J2019+37 , and study potential counterparts to explain its emission. Methods. We surveyed a region of about 6 square degrees with the Giant Metrewave Radio Telescope (GMRT) at the frequency 610 MHz. We also observed the central square degree of this survey in the near-infrared -band using the 3.5 m telescope in Calar Alto. Archival X-ray observations of some specific fields are included. VLBI observations of an interesting radio source were performed. We explored possible scenarios to produce the multi-TeV emission from MGRO J2019+37 and studied which of the sources could be the main particle accelerator. Results. We present a catalogue of 362 radio sources detected with the GMRT in the field of MGRO J2019+37 , and the results of a cross-correlation of this catalog with one obtained at near-infrared wavelengths, which contains ~3105 sources, as well as with available X-ray observations of the region. Some peculiar sources inside the ~1° uncertainty region of the TeV emission from MGRO J2019+37 are discussed in detail, including the pulsar PSR J2021+3651 and its pulsar wind nebula PWN G75.2+0.1 , two new radio-jet sources, the H II region Sh 2-104 containing two star clusters, and the radio source NVSS J202032+363158 . We also find that the hadronic scenario is the most likely in case of a single accelerator, and discuss the possible contribution from the sources mentioned above. Conclusions. Although the radio and GeV pulsar PSR J2021+3651 / AGL J2020.5+3653 and its associated pulsar wind nebula PWN G75.2+0.1 can contribute to the emission from MGRO J2019+37 , extrapolation of the GeV spectrum does not explain the detected multi-TeV flux. Other sources discussed here could contribute to the emission of the Milagro source.