Concurso internacional para la construcción de la nueva facultad de farmacia de la Universidad de Barcelona: Artemisa

Concurso internacional para la construcción de la nueva Facultad de Farmacia de la Universidad de Barcelona

Remodelació del Nou Camp del F.C. Barcelona

Proposta presentada per al Concurs de Remodelació del Nou Camp del Futbol Club Barcelona.

GalaxyDefenders: desenvolupament d'un side-scrolling shooter per iOS

Aquest projecte neix del interés personal de l’autor per a la indústria dels videojocs. El principal objectiu de l’aplicació és esdevenir un joc complet mitjançant l’ús de tècniques clàssicament empleades en el desenvolupament de jocs en dues dimensions de manera que la experiència i tècniques adquirides sigui el més reutilitzable possible.

Esport extraescolar i la utilització de les TIC i els jocs electrònics modifiquen la força de prensió de la mà?

L'objectiu del nostre estudi va ser conèixer si l'esport extraescolar i el temps dedicat setmanalment a les tecnologies de la informació i la comunicació (TIC) i jocs electrònics, tenen influència en el desenvolupament de la força de prensió de la mà i avantbraç en nens entre els 14 i 16 anys. Es va realitzar un estudi observacional de disseny transversal. La població objecte d'estudi van ser 39 nens de segon cicle de l'ESO. L'activitat física extraescolar i el temps dedicat setmanalment a les TIC i als jocs electrònics es van recollir mitjançant qüestionaris. Es va utilitzar el test d'handgrip per a la valoració de la força màxima voluntària de la mà i avantbraç del costat dominant. L'edat i la força de la mà dominant estan associades de forma estadísticament significativa, la força màxima voluntària (F=5,86; p=0,006) i el valor mig de la força sostinguda per sobre del 60% (F=4,5; p=0,02). A l'analitzar el grau d'activitat física (Kcal/setmana) respecte a la força màxima voluntària (r= 0,07; p= 0,716) i força sostinguda per sobre del 60% (r= 0,30; p= 0,09) observem una associació feble positiva i no estadísticament significativa. Si analitzem les hores setmanes TIC en relació a la força màxima voluntària observem una associació molt feble i no estadísticament significativa. La força de prensió de la mà en escolars està relacionada de forma positiva i estadísticament significativa amb l'edat i el pes corporal. No es relaciona amb el nivell d'activitat física i les hores dedicades a les TIC.

Empresas, instituciones y red social: la Compañía Hispanoamericana de Electricidad (CHADE) entre Barcelona y Buenos Aires

En este trabajo se presenta la vinculación entre la Casa de América de Barcelona y la Compañía Hispanoamericana de Electricidad (CHADE) en Buenos Aires a través del estudio de tres momentos: primero, la fundación de la asociación y la presencia de Francisco Cambó en el Centro Jurídico Iberoamericano; segundo, la fundación de la CHADE para salvar los capitales alemanes del pago de reparaciones económicas a los Aliados por su participación en la Primera Guerra Mundial; y tercero, la conversión de la asociación americanista barcelonesa en Instituto de Economía Americana (IDEA)-Casa de América para reforzar su naturaleza internacional en consonancia con la Sociedad de Naciones, así como el declive de la asociación por la interrupción de remesas de capital del Cono Sur que llegaban a Barcelona en forma de subsidios para la asociación americanista.

A photometric analysis of the Cepheus OB3 region

Results are presented on Stromgren-Crawford uvby-beta photometry carried out at Calar Alto (Spain) for 45 stars in the Cepheus OB3 region covering an apparent area of 6 deg x 6 deg. The relationship of these stars with the association is examined. Three of these stars (BD +62 deg 2114, BD +62 deg 2152, and BD +62 deg 2156) are identified as members of this association, while two more (BD +64 deg 1714 and BD +64 deg 1717) are classified as possible members. It is noted that intrinsic colors and absolute magnitudes of member stars are consistent with the hypothesis of Blaauw (1964) and Garmany (1973) of the existence of two subgroups with different evolutionary phases.

Photometric and spectroscopic survey of the cluster of galaxies Abell A2218

We present new photometric and spectroscopic observations of objects in the field of the cluster of galaxies Abell 2218. The photometric survey, centered on the cluster core, extends to a field of about 4 x 4 arcmin. It was performed in 5 bands (B,g,r,i and z filters). This sample, which includes 729 objects, is about three times larger than the survey made by Butcher and collaborators (Butcher et al., 1983, Butcher and Oemler, 1984) in the same central region of the field. Only 228 objects appear in both catalogues since our survey covers a smaller region. The spectral range covered by our filters is wider and the photometry is much deeper, up to magnitude 27 in r. The spectroscopic survey concerns 66 objects, on a field comparable to that of Butcher and collaborators. From our observations we calculate the mean redshift of the cluster, 0.1756, and its velocity dispersion, 1370 km/s. The spectral types are determined for many galaxies in the sample by comparing their spectra with synthetic ones from Rocca-Volmerange and Guiderdoni (1988).

Estimation of the extreme flash flood evolution in Barcelona county from 1351 to 2005

Every year, flash floods cause economic losses and major problems for undertaking daily activity in the Catalonia region (NE Spain). Sometimes catastrophic damage and casualties occur. When a long term analysis of floods is undertaken, a question arises regarding the changing role of the vulnerability and the hazard in risk evolution. This paper sets out to give some information to deal with this question, on the basis of analysis of all the floods that have occurred in Barcelona county (Catalonia) since the 14th century, as well as the flooded area, urban evolution, impacts and the weather conditions for any of most severe events. With this objective, the identification and classification of historical floods, and characterisation of flash-floods among these, have been undertaken. Besides this, the main meteorological factors associated with recent flash floods in this city and neighbouring regions are well-known. On the other hand, the identification of rainfall trends that could explain the historical evolution of flood hazard occurrence in this city has been analysed. Finally, identification of the influence of urban development on the vulnerability to floods has been carried out. Barcelona city has been selected thanks to its long continuous data series (daily rainfall data series, since 1854; one of the longest rainfall rate series of Europe, since 1921) and for the accurate historical archive information that is available (since the Roman Empire for the urban evolution). The evolution of flood occurrence shows the existence of oscillations in the earlier and later modern-age periods that can be attributed to climatic variability, evolution of the perception threshold and changes in vulnerability. A great increase of vulnerability can be assumed for the period 1850¿1900. The analysis of the time evolution for the Barcelona rainfall series (1854¿2000) shows that no trend exists, although, due to changes in urban planning, flash-floods impact has altered over this time. The number of catastrophic flash floods has diminished, although the extraordinary ones have increased.

An observational study of the 7 September 2005 Barcelona tornado outbreak

This paper presents an observational study of the tornado outbreak that took place on the 7 September 2005 in the Llobregat delta river, affecting a densely populated and urbanised area and the Barcelona International airport (NE Spain). The site survey confirmed at least five short-lived tornadoes. Four of them were weak (F0, F1) and the other one was significant (F2 on the Fujita scale). They started mostly as waterspouts and moved later inland causing extensive damage estimated in 9 million Euros, three injured people but fortunately no fatalities. Large scale forcing was provided by upper level diffluence and low level warm air advection. Satellite and weather radar images revealed the development of the cells that spawned the waterspouts along a mesoscale convergence line in a highly sheared and relatively low buoyant environment. Further analysis indicated characteristics that could be attributed indistinctively to non-supercell or to mini-supercell thunderstorms.

Exploring the connection between the stellar wind and the non-thermal emission in LS 5039

Context.LS 5039 has been observed with several X-ray instruments so far showing quite steady emission in the long term and no signatures of accretion disk. The source also presents X-ray variability at orbital timescales in flux and photon index. The system harbors an O-type main sequence star with moderate mass-loss. At present, the link between the X-rays and the stellar wind is unclear. Aims.We study the X-ray fluxes, spectra, and absorption properties of LS 5039 at apastron and periastron passages during an epoch of enhanced stellar mass-loss, and the long term evolution of the latter in connection with the X-ray fluxes. Methods.New XMM-Newton observations were performed around periastron and apastron passages in September 2005, when the stellar wind activity was apparently higher. April 2005 Chandra observations on LS 5039 were revisited. Moreover, a compilation of H EW data obtained since 1992, from which the stellar mass-loss evolution can be approximately inferred, was carried out. Results.XMM-Newton observations show higher and harder emission around apastron than around periastron. No signatures of thermal emission or a reflection iron line indicating the presence of an accretion disk are found in the spectrum, and the hydrogen column density () is compatible with being the same in both observations and consistent with the interstellar value. 2005 Chandra observations show a hard X-ray spectrum, and possibly high fluxes, although pileup effects preclude conclusive results from being obtained. The H EW shows yearly variations of 10%, and does not seem to be correlated with X-ray fluxes obtained at similar phases, unlike what is expected in the wind accretion scenario. Conclusions.2005 XMM-Newton and Chandra observations are consistent with 2003 RXTE/PCA results, namely moderate flux and spectral variability at different orbital phases. The constancy of the seems to imply that either the X-ray emitter is located at 1012 cm from the compact object, or the density in the system is 3 to 27 times smaller than that predicted by a spherical symmetric wind model. We suggest that the multiwavelength non-thermal emission of LS 5039 is related to the observed extended radio jets and is unlikely to be produced inside the binary system.