Multiwavelength observations of the black hole candidate 1E 1740.7-2942

Observations of the Galactic center region black hole candidate 1E 1740.7-2942 have been carried out using the Caltech Gamma-Ray Imaging Payload (GRIP), the Röntgensatellit (ROSAT) and the Very Large Array (VLA). These multiwavelength observations have helped to establish the association between a bright emitter of hard X-rays and soft γ-rays, the compact core of a double radio jet source, and the X-ray source, 1E 1740.7-2942. They have also provided information on the X-ray and hard X-ray spectrum.

The Galactic center region was observed by GRIP during balloon flights from Alice Springs, NT, Australia on 1988 April 12 and 1989 April 3. These observations revealed that 1E 1740.7-2942 was the strongest source of hard X-rays within ~10° of the Galactic center. The source spectrum from each flight is well fit by a single power law in the energy range 35-200 keV. The best-fit photon indices and 100 keV normalizations are: γ = (2.05 ± 0.15) and K_(100) = (8.5 ± 0.5) x 10^(-5) cm^(-2) s^(-1) keV^(-1) and γ = (2.2 ± 0.3) and K_(100) = (7.0 ± 0.7) x 10^(-5) cm^(-2) s^(-1) keV^(-1) for the 1988 and 1989 observations respectively. No flux above 200 keV was detected during either observation. These values are consistent with a constant spectrum and indicate that 1E 1740.7-2942 was in its normal hard X-ray emission state. A search on one hour time scales showed no evidence for variability.

The ROSAT HRI observed 1E 1740.7-2942 during the period 1991 March 20-24. An improved source location has been derived from this observation. The best fit coordinates (J2000) are: Right Ascension = 17^h43^m54^s.9, Declination = -29°44'45".3, with a 90% confidence error circle of radius 8".5. The PSPC observation was split between periods from 1992 September 28- October 4 and 1993 March 23-28. A thermal bremsstrahlung model fit to the data yields a column density of N_H = 1.12^(+1.51)_(0.18) x cm^(-2) , consistent with earlier X- ray measurements.

We observed the region of the Einstein IPC error circle for 1E 1740.7-2942 with the VLA at 1.5 and 4.9 GHz on 1989 March 2. The 4.9 GHz observation revealed two sources. Source 'A', which is the core of a double aligned radio jet source (Mirabel et al. 1992), lies within our ROSAT error circle, further strengthening its identification with 1E 1740.7-2942.

Physical investigations of small particles : (I) aerosol particle charging and flux enhancement and (II) whispering gallery mode sensing

Part I

Particles are a key feature of planetary atmospheres. On Earth they represent the greatest source of uncertainty in the global energy budget. This uncertainty can be addressed by making more measurement, by improving the theoretical analysis of measurements, and by better modeling basic particle nucleation and initial particle growth within an atmosphere. This work will focus on the latter two methods of improvement.

Uncertainty in measurements is largely due to particle charging. Accurate descriptions of particle charging are challenging because one deals with particles in a gas as opposed to a vacuum, so different length scales come into play. Previous studies have considered the effects of transition between the continuum and kinetic regime and the effects of two and three body interactions within the kinetic regime. These studies, however, use questionable assumptions about the charging process which resulted in skewed observations, and bias in the proposed dynamics of aerosol particles. These assumptions affect both the ions and particles in the system. Ions are assumed to be point monopoles that have a single characteristic speed rather than follow a distribution. Particles are assumed to be perfect conductors that have up to five elementary charges on them. The effects of three body interaction, ion-molecule-particle, are also overestimated. By revising this theory so that the basic physical attributes of both ions and particles and their interactions are better represented, we are able to make more accurate predictions of particle charging in both the kinetic and continuum regimes.

The same revised theory that was used above to model ion charging can also be applied to the flux of neutral vapor phase molecules to a particle or initial cluster. Using these results we can model the vapor flux to a neutral or charged particle due to diffusion and electromagnetic interactions. In many classical theories currently applied to these models, the finite size of the molecule and the electromagnetic interaction between the molecule and particle, especially for the neutral particle case, are completely ignored, or, as is often the case for a permanent dipole vapor species, strongly underestimated. Comparing our model to these classical models we determine an “enhancement factor” to characterize how important the addition of these physical parameters and processes is to the understanding of particle nucleation and growth.

Part II

Whispering gallery mode (WGM) optical biosensors are capable of extraordinarily sensitive specific and non-specific detection of species suspended in a gas or fluid. Recent experimental results suggest that these devices may attain single-molecule sensitivity to protein solutions in the form of stepwise shifts in their resonance wavelength, \lambda_{R}, but present sensor models predict much smaller steps than were reported. This study examines the physical interaction between a WGM sensor and a molecule adsorbed to its surface, exploring assumptions made in previous efforts to model WGM sensor behavior, and describing computational schemes that model the experiments for which single protein sensitivity was reported. The resulting model is used to simulate sensor performance, within constraints imposed by the limited material property data. On this basis, we conclude that nonlinear optical effects would be needed to attain the reported sensitivity, and that, in the experiments for which extreme sensitivity was reported, a bound protein experiences optical energy fluxes too high for such effects to be ignored.

Una aproximación psicosocial al conflicto vasco. Construyendo la paz en espacio abierto

450 p.

Adaptaciones literarias dirigidas al público infanto-juvenil. El caso del Lazarillo de Tormes.

[SPA] Múltiples son las formas en las que se materializa la intertextualidad, entendida como el conjunto de relaciones que se establecen entre obras diferentes. Una de estas expresiones intertextuales es la adaptación literaria de los clásicos, que transforma textos originariamente dirigidos al público adulto en obras para el joven lector. Tomando como ejemplo diversas versiones infantiles del Lazarillo de Tormes, se han analizado las estrategias empleadas en su adaptación y se ha reflexionado sobre las profundas modificaciones a las que se somete el hipotexto. La exploración de esta temática ha permitido hacer visible la imagen desfigurada que, de forma consciente o inconsciente, la Literatura Infantil y Juvenil transmite en ocasiones de los clásicos universales.

The ^(26)Al(p,γ)^(27)Si reaction : stellar origins of galactic ^(26)Al

To explain the ^(26)Mg isotopic anomaly seen in meteorites (^(26)Al daughter) as well as the observation of 1809-keV γ rays in the interstellar medium (live decay of 26Al) one must know, among other things, the destruction rate of ^(26)Al. Properties of states in ^(27)Si just above the ^(26)Al + p mass were investigated to determine the destruction rate of ^(26)Al via the ^(26)Al(p,γ)^(27)Si reaction at astrophysical temperatures.

Twenty micrograms of ^(26)Al were used to produce two types of Al_2O_3 targets by evaporation of the oxide. One was onto a thick platinum backing suitable for (p,γ) work, and the other onto a thin carbon foil for the (^3He,d) reaction.

The ^(26)Al(p,γ)^(27)Si excitation function, obtained using a germanium detector and voltage-ramped target, confirmed known resonances and revealed new ones at 770, 847, 876, 917, and 928 keV. Possible resonances below the lowest observed one at E_p = 286 keV were investigated using the ^(26)Al(^3He,d)^(27)Si proton-transfer reaction. States in 27Si corresponding to 196- and 286-keV proton resonances were observed. A possible resonance at 130 keV (postulated in prior work) was shown to have a strength of wγ less than 0.02 µeV.

By arranging four large Nal detector as a 47π calorimeter, the 196-keV proton resonance, and one at 247 keV, were observed directly, having wγ = 55± 9 and 10 ± 5 µeV, respectively.

Large uncertainties in the reaction rate have been reduced. At novae temperatures, the rate is about 100 times faster than that used in recent model calculations, casting some doubt on novae production of galactic ^(26)Al.

Diseño y puesta en practica de una intervención psicoeducativa en relación al logro de un autoconcepto ajustado.

El autoconcepto es una pieza esencial para el desarrollo adecuado del individuo, por lo que en este trabajo se elabora y aplica una intervención en relación al logro de un autoconcepto ajustado. Para ello, se llevan a cabo una serie de dinámicas en un grupo-clase y periodo de tiempo específicos. Asimismo, se utilizan una serie de instrumentos de medida previa y posteriormente a la intervención, con el objetivo de evaluar las posibles variaciones en lo que al autoconcepto de los alumnos respecta. Finalmente, se concluyen ciertas variaciones que más que reflejar grandes cambios en el autoconcepto del alumnado, indican la importancia y posible eficacia de programas que dirigen su atención a dicho constructo

Utilidad de la biblioteca escolar como recurso al servicio del proyecto educativo

RESUMEN: En este trabajo se plasma la transcendencia que tiene la lectura en el desarrollo integral de las personas. Del mismo modo, consideramos fundamental que se fomente la lectura en la escuela desde la etapa de infantil. El supuesto de nuestro trabajo es que la escuela cuenta con un espacio que contiene todo lo necesario para fomentar el hábito lector: la biblioteca escolar. Para nuestra investigación nos hemos acercado a un centro escolar de Amorebieta (Bizkaia) para conocer si el funcionamiento de las bibliotecas escolares se realiza siguiendo los patrones que se consideran adecuados desde la literatura especializada en el tema.

Itinerarios, del espacio al plano. Descubriendo el camino de la escuela al metro.

Resumen: Este Trabajo de Fin de Grado tiene como objeto de estudio los recorridos en el espacio a través de su representación en el plano. Presentamos una propuesta educativa basada en los principios de la enseñanza matemática realista. Utilizando como contexto los recorridos en el entorno de la escuela, matematizamos un contexto en el que los niños y niñas viven y experimentan, diseñando tareas y actividades que nos permitieron relacionar los procesos matemáticos con los contenidos curriculares de esta etapa. La implementación en el centro en el que realizábamos las prácticas nos permitió analizar los resultados obtenidos que presentamos en las conclusiones.

Actitudes frente al peso corporal de estudiantes de la Universidad del País Vasco

[ES] La presión que la sociedad ejerce sobre sus miembros hace que , exista un tendencia generalizada a la excesiva preocupación por el peso y la apariencia física. Se estudiaron las actitudes frente al peso de 526 estudiantes, 158 hombres y 368 mujeres. Muestran un deseo de ser más delgados de lo que son aunque consideran su peso menor al saludable.

Análisis de sensibilidad en los procedimientos de calibración de robots de cinemática paralela Aplicación al mecanismo 5R

[ES]Este proyecto investigador tiene como objetivo el ayudar con la calibración del mecanismo de cinco pares de rotación montado en el taller de Ingeniería Mecánica de la ETSI de Bilbao. En primer lugar se estudiarán los algoritmos de optimización prestando especial atención a la comparativa entre Levenberg-Marquart y Gauss-Newton. Se realizarán estudios en Matlab para concluir cuál de los dos es más eficaz tanto en rapidez como en precisión. El que sea más adecuado se implementará en un programa para la calibración del mecanismo 5R. En segundo lugar se estudiarán los índices de observabilidad. Los estudios que se han realizado sobre ellos hasta ahora son poco concluyentes asique se intentará aclarar su utilidad y determinar cuál es el que conviene utilizar en este caso. Para ello se deberá programar la resolución del problema cinemático inverso. Por último se presentarán los resultados y las conclusiones correspondientes. Se propondrá también un plan de desarrollo de una línea de investigación futura que partirá con este trabajo como base.

Criterios y parametros de desarrollo sostenible aplicables al planeamiento urbano y su ejecución

[ES]Todo aquello, real o conceptual, que podamos imaginar aparece una vez que tiene un soporte físico. La insostenibilidad proviene del uso desaforado de los recursos naturales para satisfacer los deseos del presente, que lleva a una menor disponibilidad de los mismos en el largo plazo. Esto ocurre porque los flujos de materia y energía se modifican y también lo hacen los agentes que en ellos participan. La hoja de ruta para alcanzar la sostenibilidad es, por una parte, ir promoviendo un cambio de conciencia en el seno de la sociedad y a la vez, aplicar soluciones técnicas que lleven el sello de la sostenibilidad. Este cambio, es una actuación conjunta y necesita de la participación de todos los seres humanos para tener esperanzas de éxito. La ciudad, ecológicamente, es un agujero negro e incluye no sólo lo que es, sino también lo que necesita para mantenerse tal y como es. La planificación urbana ecológica intenta aunar lo urbano y lo sostenible, ya que tiene como propósito proponer áreas donde los asentamientos humanos sean favorables y produzcan menos repercusiones negativas en el entorno. Para lograrlo, energía, materiales constructivos, agua, residuos, zonas verdes, comunidad y la incidencia en la legislación son ámbitos en los que el planeamiento urbano sostenible debe actuar. Los seres humanos somos los poseedores de nuestro destino. Los resultados son consecuencia de las acciones. Si algo ocurre es porque nuestras acciones han sido las elegidas para que así sea.

Part I. Energy straggling of ^4He below 2.0 MeV in Al, Ni, Au and Pt. Part II. Studies of the Ti-W metallization system on Si

Part I.

In recent years, backscattering spectrometry has become an important tool for the analysis of thin films. An inherent limitation, though, is the loss of depth resolution due to energy straggling of the beam. To investigate this, energy straggling of ⁴He has been measured in thin films of Ni, Al, Au and Pt. Straggling is roughly proportional to square root of thickness, appears to have a slight energy dependence and generally decreases with decreasing atomic number of the adsorber. The results are compared with predictions of theory and with previous measurements. While Ni measurements are in fair agreement with Bohr's theory, Al measurements are 30% above and Au measurements are 40% below predicted values. The Au and Pt measurements give straggling values which are close to one another.

Part II.

MeV backscattering spectrometry and X-ray diffraction are used to investigate the behavior of sputter-deposited Ti-W mixed films on Si substrates. During vacuum anneals at temperatures near 700°C for several hours, the metallization layer reacts with the substrate. Backscattering analysis shows that the resulting compound layer is uniform in composition and contains Ti, Wand Si. The Ti:W ratio in the compound corresponds to that of the deposited metal film. X-ray analyses with Reed and Guinier cameras reveal the presence of the ternary Ti_xW_(1-x)Si₂ compound. Its composition is unaffected by oxygen contamination during annealing, but the reaction rate is affected. The rate measured on samples with about 15% oxygen contamination after annealing is linear, of the order of 0.5 Å per second at 725°C, and depends on the crystallographic orientation of the substrate and the dc bias during sputter-deposition of the Ti-W film.

Au layers of about 1000 Å thickness were deposited onto unreacted Ti-W films on Si. When annealed at 400°C these samples underwent a color change,and SEM micrographs of the samples showed that an intricate pattern of fissures which were typically 3µm wide had evolved. Analysis by electron microprobe revealed that Au had segregated preferentially into the fissures. This result suggests that Ti-W is not a barrier to Au-Si intermixing at 400°C.