Análisis de los métodos de transporte en la localización de empresas y su aplicación en la incertidumbre

En el presente trabajo se pretende dar una visión general de los métodos más conocidos de resolución del problema del transporte, introduciendo el método del coste mínimo escalonado en situación de certeza, comparándolos entre sí, así como su aplicación en el campo de la incertidumbre, todo ello, mediante un ejemplo práctico.

Del Benchmarking al outsourcing estratégico

El presente trabajo pretende dar una visión particular del benchmarking y del outsourcing. El primero, como instrumento para conocer el perfil estratégico de la empresa y el segundo, como alternativa en el caso que la organización no pueda, por razones de coste, mejorar sus puntos débiles con las mejores prácticas de otra empresa.

The use of micro-XRD for the study of glaze color decorations

The compounds responsible for the colours and decorations in glass and glazed ceramics include: colouring agents (transition metal ions), pigments (micro-and nano-precipitates of compounds that either do not dissolve or recrystallize in the glassy matrix) and opacifiers (microcrystalline compounds with high light scattering capability). Their composition, structure and range of stability are highly dependent not only on the composition but also on the procedures followed to obtain them. Chemical composition of the colorants and crystallites may be obtained by means of SEM-EDX and WDX. Synchrotron Radiation micro-X-ray Diffraction has a small beam size adequate (10 to 50 microns footprint size) to obtain the structural information of crystalline compounds and high brilliance, optimal for determining the crystallites even when present in low amounts. In addition, in glass decorations the crystallites often appear forming thin layers (from 10 to 100 micrometers thick) and they show a depth dependent composition and crystal structure. Their nature and distribution across the glass/glazes decorations gives direct information on the technology of production and stability and may be related to the color and appearance. A selection of glass and glaze coloring agents and decorations are studied by means of SR-micro- XRD and SEM-EDX including: manganese brown, antimony yellow, red copper lusters and cobalt blue. The selection includes Medieval (Islamic, and Hispano Moresque) and renaissance tin glazed ceramics from the 10th to the 17th century AD.

La medina andalusina de Lleida en el segle XI: identitat i societat

La ciutat a Alandalús és l’espai hegemònic del poder públic emiral i posteriorment califal. Partint de la ciutat de Lleida, analitzem la evolució des del segle VIII fins al segle XI de la consolidació dels espais urbans com a representants del poder. Talment, aquests, capitalitzen els districtes o cores, mitjançant una xarxa de ciutats i fortificacions que li donen cohesió interna. Paral∙lelament, es vertebra i s’envigoritza una societat urbana partint d’elements comuns d’identitat i d’un discurs ideològic afí a la dinastia Omeia. La “gent de la ciutat” repre‐senten una part de la societat andalu‐sina, d’arrels hispano‐visigodes, i alhora, assumeixen l’hegemonia cultural de l’Islam, tot convivint en la nova realitat político‐social.

Deep radio images of the HEGRA and Whipple TeV sources in the Cygnus OB2 region.

The modern generation of Cherenkov telescopes has revealed a new population of gamma-ray sources in the Galaxy. Some of them have been identified with previously known X-ray binary systems while other remain without clear counterparts a lower energies. Our initial goal here was reporting on extensive radio observations of the first extended and yet unidentified source, namely TeV J2032+4130. This object was originally detected by the HEGRA telescope in the direction of the Cygnus OB2 region and its nature has been a matter of debate during the latest years. The situation has become more complex with the Whipple and MILAGRO telescopes new TeV detections in the same field which could be consistent with the historic HEGRA source, although a different origin cannot be ruled out. Aims.We aim to pursue our radio exploration of the TeV J2032+4130 position that we initiated in a previous paper but taking now into account the latest results from new Whipple and MILAGRO TeV telescopes. The data presented here are an extended follow up of our previous work. Methods.Our investigation is mostly based on interferometric radio observations with the Giant Metre Wave Radio Telescope (GMRT) close to Pune (India) and the Very Large Array (VLA) in New Mexico (USA). We also conducted near infrared observations with the 3.5 m telescope and the OMEGA2000 camera at the Centro Astronómico Hispano Alemán (CAHA) in Almería (Spain). Results.We present deep radio maps centered on the TeV J2032+4130 position at different wavelengths. In particular, our 49 and 20 cm maps cover a field of view larger than half a degree that fully includes the Whipple position and the peak of MILAGRO emission. Our most important result here is a catalogue of 153 radio sources detected at 49 cm within the GMRT antennae primary beam with a full width half maximum (FWHM) of 43 arc-minute. Among them, peculiar sources inside the Whipple error ellipse are discussed in detail, including a likely double-double radio galaxy and a one-sided jet source of possible blazar nature. This last object adds another alternative counterpart possibility to be considered for both the HEGRA, Whipple and MILAGRO emission. Moreover, our multi-configuration VLA images reveal the non-thermal extended emission previously reported by us with improved angular resolution. Its non-thermal spectral index is also confirmed thanks to matching beam observations at the 20 and 6 cm wavelengths.

Mercado del libro y empresas editoriales entre el Centenario de Independencias y la Guerra Civil española: la editorial Sudamericana

[spa]Las estrategias comerciales de los libreros y editores españoles para desembarcar en los mercados americanos son analizadas en un contexto signado por las tendencias americanistas en el plano político y las iniciativas regeneracionistas en el económico durante el periodo que va del Centenario de las Independencias hasta la Guerra Civil española. Se abordan algunas de las políticas empresariales editoriales implementadas en Cataluña, el liderazgo ejercido por esta región como epicentro del proyecto hispano, y finalmente las condiciones que permitieron la creación de la editorial Sudamericana en Buenos Aires ante la inminencia del triunfo franquista. Los ejes de estudio son las estrategias editoriales y comerciales; el peso de las asociaciones y corporaciones patronales del libro; y los vínculos tejidos con el sector intelectual argentino en las primeras décadas del siglo XX a través de delegaciones consulares, instituciones culturales y cámaras españolas de comercio.

Candidate counterparts to the soft gamma-ray flare in the direction od LSI+61303

A short duration burst reminiscent of a soft gamma-ray repeater/anomalous X-ray pulsar behaviour was detected in the direction of LS I +61 303 by the Swift satellite. While the association with this well known gamma-ray binary is likely, a different origin cannot be excluded. Aims. We explore the error box of this unexpected flaring event and establish the radio, near-infrared and X-ray sources in our search for any peculiar alternative counterpart. Methods. We carried out a combined analysis of archive Very Large Array radio data of LS I +61 303 sensitive to both compact and extended emission. We also reanalysed previous near infrared observations with the 3.5 m telescope of the Centro Astronómico Hispano Alemán and X-ray observations with the Chandra satellite. Results. Our deep radio maps of the LS I +61 303 environment represent a significant advancement on previous work and 16 compact radio sources in the LS I +61 303 vicinity are detected. For some detections, we also identify near infrared and X-ray counterparts. Extended emission features in the field are also detected and confirmed. The possible connection of some of these sources with the observed flaring event is considered. Based on these data, we are unable to claim a clear association between the Swift-BAT flare and any of the sources reported here. However, this study represents the most sophisticated attempt to determine possible alternative counterparts other than LS I +61 303.