A microquasar model applied to unidentified gamma-ray sources

Among unidentified gamma-ray sources in the galactic plane, there are some that present significant variability and have been proposed to be high-mass microquasars. To deepen the study of the possible association between variable low galactic latitude gamma-ray sources and microquasars, we have applied a leptonic jet model based on the microquasar scenario that reproduces the gamma-ray spectrum of three unidentified gamma-ray sources, 3EG J1735-1500, 3EG J1828+0142 and GRO J1411-64, and is consistent with the observational constraints at lower energies. We conclude that if these sources were generated by microquasars, the particle acceleration processes could not be as efficient as in other objects of this type that present harder gamma-ray spectra. Moreover, the dominant mechanism of high-energy emission should be synchrotron self-Compton (SSC) scattering, and the radio jets may only be observed at low frequencies. For each particular case, further predictions of jet physical conditions and variability generation mechanisms have been made in the context of the model. Although there might be other candidates able to explain the emission coming from these sources, microquasars cannot be excluded as counterparts. Observations performed by the next generation of gamma-ray instruments, like GLAST, are required to test the proposed model.

Optical spectroscopy of microquasar candidates at low Galactic latitudes

We report optical spectroscopic observations of a sample of 6 low-galactic latitude microquasar candidates selected by cross-identification of X-ray and radio point source catalogs for |b|<5 degrees. Two objects resulted to be of clear extragalactic origin, as an obvious cosmologic redshift has been measured from their emission lines. For the rest, none exhibits a clear stellar-like spectrum as would be expected for genuine Galactic microquasars. Their featureless spectra are consistent with being extragalactic in origin although two of them could be also highly reddened stars. The apparent non-confirmation of our candidates suggests that the population of persistent microquasar systems in the Galaxy is more rare than previously believed. If none of them is galactic, the upper limit to the space density of new Cygnus X-3-like microquasars within 15 kpc would be 1.1\times10^{-12} per cubic pc. A similar upper limit for new LS 5039-like systems within 4 kpc is estimated to be 5.6\times10^{-11} per cubic pc.

LS 5039: A runaway microquasar ejected from the galactic plane

We have compiled optical and radio astrometric data of the microquasar LS 5039 and derived its proper motion. This, together with the distance and radial velocity of the system, allows us to state that this source is escaping from its own regional standard of rest, with a total systemic velocity of about 150 km/s and a component perpendicular to the galactic plane larger than 100 km/s. This is probably the result of an acceleration obtained during the supernova event that created the compact object in this binary system. We have computed the trajectory of LS 5039 in the past, and searched for OB associations and supernova remnants in its path. In particular, we have studied the possible association between LS 5039 and the supernova remnant G016.8-01.1, which, despite our efforts, remains dubious. We have also discovered and studied an HI cavity in the ISM, which could have been created by the stellar wind of LS 5039 or by the progenitor of the compact object in the system. Finally, in the symmetric supernova explosion scenario, we estimate that at least 17 solar masses were lost in order to produce the high eccentricity observed. Such a mass loss could also explain the observed runaway velocity of the microquasar.

On the Hall effect in polycrystalline semiconductors

Some problems involved in the interpretation of Hall‐effect measurements in polycrystalline semiconductors have not been resolved, especially when the contribution of the boundaries is appreciable. Using the Herring theory of transport properties in inhomogeneous semiconductors, we present an alternative interpretation to that previously proposed. This model permits the calculation of the Hall coefficient under general conditions.

La Cova des Pas de Ferreries: notícia de la seva troballa

Durant la primavera del 2005, tres espeleòlegs es varen endinsar al barranc de Trebalúger, a prop de Ferreries, al sud-est de l"illa de Menorca. El seu objectiu era el barranc; l"havien vist feia unes quantes setmanes i no podien deixar passar aquell forat, de difícil accés. No sabien que estaven a punt de fer una de les troballes més extraordinàries de la prehistòria menorquina. Varen assegurar les cordes al cim de la paret i, tot fent un ràpel de trenta-cinc metres, accediren a un petit forat, veí de la cova a la qual volien arribar. Des d"allà varen haver de reptar, penjats de l"espadat, per una mena de graó estret o postada, un pas obligat per arribar-hi, que acabaria donant nom a la petita cova. Quan varen accedir al graó d"entrada ja havien decidit que allò seria la cova des Pas.

Els prats de l'alianÇa Xerobromion als Pirineus Catalans

En este trabajo se intenta dar una visión sintética de las comunidades de la alianza Xerobromion conocidas hasta el momento de los Pirineos catalanes. Se distinguen en dicho territorio nueve asociaciones distintas, cinco de ellas ya descritas con anterioridad (Koelerio-Avenuletum mirandanae, Achilleo-Dichanthietum ischaemi,. Teucrio (pyrenaici )-Brometum, Lino (viscosi)-Brometum, Koelerio-Globularietum punctatae) y las cuatro restantes propuestas como nuevas (Cleistogeno-Dichanthietum ischaemi , Teucrio (montani )-Avenuletum mirandanae, Adonido-Brometum e Irido (germanici)-Brometum). De todas ellas, y más especialmente de estas últimas, se hacen comentarios relativos a su estructura, composición florística, ecología y distribución. Además de las tablas de inventarios correspondientes a cada una de las nuevas asociaciones, se ha elaborado una tabla sintética que agrupa el total de las comunidades consideradas.

Valoración experiencial del aprendizaje tras formación virtual.

[eng] An observable study on the behaviour in the laboratory of Pharmaceutical Technology II (pharmaceutical pilot plant), with two groups of students of 3rd course (proactive aptitude and valuation of the"knowledge to do acquired") is carried out. The variable between groups is that one has realised a training (by means of self-study of an interactive application multimedia, especially designed), without tutorship on behalf the teacher in front of the other group that carried out the same training with the same material but with the guide of the teacher in the computer lab. On the one hand it is valued if there is some effect differentiator between both types of training, by means of the accounting of the correct results obtained in a previous test to the entrance in the pilot plant and by another one the valuation that the professors made responsible for the groups of practices in situ. The results demonstrate the previous hypothesis that there must not be significant differences between the groups, beyond the inherent ones to personality of the students itself (interest and personal implication by the subject). On the other hand the test for the observation in the laboratory did not facilitate the distinction of objective differences. [spa] Se lleva a cabo un estudio observacional sobre el comportamiento de los estudiantes (aptitud pro-activa y valoración del “saber hacer adquirido”) en el laboratorio de Tecnología Farmacéutica II (planta piloto farmacéutica) de dos grupos de estudiantes de 3er curso. La variable entre los dos grupos es que uno ha realizado una formación no presencial (mediante el autoestudio de una aplicación interactiva multimedia, especialmente diseñada), sin tutoría por parte del profesor, frente al otro grupo que llevó a cabo la misma formación con el mismo material pero con la guía del profesor en el aula de informática. Por una parte se valora si hay algún efecto diferenciador entre ambos tipos de formación, mediante la contabilización de los resultados correctos obtenidos en un test previo a la entrada en la planta piloto y por otro la valoración que hicieron los profesores responsables de los grupos de prácticas in situ. Los resultados demuestran la hipótesis previa de que no debían existir diferencias significativas entre los grupos, más allá de las inherentes a la propia personalidad de los estudiantes (interés e implicación personal por el tema). Por otra parte el test para la observación en el laboratorio no facilitó la distinción de diferencias objetivas.

EVN+MERLIN observations of microquasar candidates at low galactic latitudes

In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a long-term project focused on the search for new objects of this type. They performed a cross-identification between X-ray and radio catalogs under very restrictive selection criteria for sources with |b|<5 degrees, and obtained a sample of 13 radio-emitting X-ray sources. Follow-up observations of 6 of these sources with the VLA provided accurate coordinates, which were used to discover optical counterparts for all of them. We have observed these six sources with the EVN and MERLIN at 5 GHz. Five of the six objects have been detected and imaged, presenting different morphologies: one source has a two-sided jet, three sources have one-sided jets, and one source is compact. With all the presently available information, we conclude that two of the sources are promising microquasar candidates in our Galaxy.

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.

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