Paisaje e imagen: formas y herencias en la construcción cultural del territorio agrario

El sistema agrario, en sus escalas territorial, urbana y arquitectónica, es escudriñado en busca de las claves del carácter paisajístico, mediante la encuesta oral, el registro documental, la interpretación reflexiva a través del dibujo, y las técnicas cartográficas y fotogramétricas avanzadas.

Fernández Alba : Arquitectura y Urbanismo

Anteriormente publicado el 24 de mayo de 1969 en el Diario de Mallorca

La iglesia de Santiago de los españoles en Roma y su entorno entre los siglos XV y XIX. Una historia a través del dibujo

Plaza Navona representa una de las visitas obligadas de Roma, pero solo algunos advertirán en ella la presencia española en la sala de exposiciones del Instituto Cervantes o en la inmediata Libreria Española. Todavía serán menos los que se percatarán de la huella española dejada en aquella iglesia de fachada anónima situada, en el extremo sur de la plaza: la antigua iglesia de Santiago de los Españoles. La presente tesis pretende, utilizando el dibujo como guía, herramienta y fin del proceso de análisis y estudio, reconstruir el proceso de conformación y construcción de la que fue iglesia española principal, cuya fundación hace patente el destacado papel jugado por la “nación” castellana en Roma durante la Edad Media; y en torno a la que se aglutinaron las actividades religiosas, diplomáticas y financieras de los castellanos que vivieron en la actual capital italiana. Se intentará recrear en el tiempo la que es hoy la iglesia de Nuestra Señora del Sagrado Corazón, sometiéndola a una restitución gráfica disciplinada, homogénea y objetiva en la medida de lo posible de las varias etapas que la han caracterizadas, desde su fundación hasta cuando en 1878 España se deshizo de ella, ya en ruina, vendiéndola. Como nos comenta Gaetano Moroni, de todas las comunidades nacionales que se encontraban en Roma la española parece ser efectivamente una de las más rica y prestigiosa. Aunque lo que no cuenta Moroni no haya sido todavía demostrado, dicho enunciado resulta de todas formas interesante puesto que pone el acento sobre el hecho de que ya desde el siglo X parece ser habitual de ocupar y reutilizar antiguas ruinas, usándolas como base para la construcción de hospitales para los peregrinos. Esta operación se hizo particularmente frecuente sobre todo antes del Gran Jubileo de 1450: de hecho desde la primera mitad del Quattrocento se fundan distintas iglesias y hospitales nacionales para acoger y prestar una adecuada asistencia y socorro a los innumerables peregrinos que llegaban a la ciudad, edificios que se van construyendo sobre los restos de antiguos edificios de época romana. Prueba de ello es en efecto la fundación originaria de la iglesia y hospital de los Españoles que, parte del conjunto de edificios que compone la Plaza Navona, situada en el corazón de Campo Marzio y cuya posición y forma corresponden a la del antiguo Estadio de Domiciano, y que ahora es en sus dimensiones, en su imagen arquitectónica y en su consistencia material, el resultado de la definición proyectual y de las transformaciones que se llevaron a cabo sobre lo que quedaba del antiguo templo español del siglo XV, entre finales del ‘800 y los años 30 del siglo XX . Transformaciones devastadoras, huellas grabadas o canceladas que encuentran una justificación en los acontecimientos históricos reflejados en el patrimonio urbano. El análisis de todas las fuentes permite trazar, si no la totalidad, buena parte de las modificaciones que la antigua iglesia de Santiago ha sufrido. La construcción del templo se puede dividir en tres momentos decisivos: una primera etapa de fundación en 1450-1478 en la que la iglesia tenía fachada y entrada en via de la Sapienza, hoy Corso Rinascimento; una segunda de significativa ampliación hacia Plaza Navona con una nueva fachada monumental hacia ese espacio público en 1496-1500; y una última importante ampliación entre 1525-1526, llevada a cabo por el arquitecto Antonio da Sangallo el Joven. Tras la intensa vida del templo, en el siglo XVIII, éste cae en ruina y finalmente es vendido en 1878 a la orden de los misioneros franceses de Nuestra Señora del Sagrado Corazón que la reconvierten en iglesia reformando totalmente el conjunto en 1881, según proyecto de Luca Carimini. En 1936, en plena fase de rectificación de trazados urbanos por obra del régimen fascista, según proyecto de Arnaldo Foschini, se mutila su extremidad hacia vía de la Sapienza dejando su estado tal y como se contempla en la actualidad. ABSTRACT The objective of this thesis is the reconstruction of the design and edification process -using drawings and sketches as a guide, tool and the end of the analytical process- of a church which was once the preeminent Spanish church in medieval Rome, known today as Nostra Signora del Sacro Cuore (Our Lady of the Sacred Heart). The founding of this church illustrates the important role held by the Castillian “nation” in Rome during the Middle Ages. It was the focal point of all the religious, diplomatic and economic activities of the Castillian community residing in today’s Italian capital. The aim of this proyect is a recreation the church in time by submitting it to a disciplined, homogenous and objective graphic restitution of the various stages most characteristic the temple, starting from its foundation until 1878 when, in a state of ruins, the church was finally sold off by Spain. Gaetano Moroni once commented that of all the international communities found in Rome, the Spanish community seemed to be one of the wealthiest and most prestigious. Such a statement proves interesting as it emphasizes that starting in the 10th century we see there was a widespread custom of occupying and reusing old ruins for use as the bases of new constructions of hospitals for pilgrims. This custom became especially frequent just before the Jubilee Year of 1450: in fact, in the first half of the Quattrocento we see the founding of many different national churches and hospitals which provided shelter and care to the countless pilgrims arriving in the city, buildings which were constructed on top of the ruins of ancient buildings left over from Roman times. Proof of this is the original foundation of the Spanish church and hospital forming part of the Piazza Navona, built upon and following the outline of the Stadium of Domitian, in the heart of Campo Marzio. Now, in its dimensions, its architectural image and its material substance, it represents the predominant result of the planning definitions and the transformations which affected the old 15th-century Spanish temple. Ocurring between the end of the 19th century and the 1930s, the transformations were devastating, erasing original peculiarities and engraving new ones, transformations made justifiable by the historical events reflected in its urban environs. Analyzing all sources allows us to trace, even if not in entirety, still a sizeable portion of the modifications undergone by the old Church of Saint James. The construction of the temple can be divided into three decisive moments: its foundation, from 1450 to 1478, when the church’s façade and main door looked out on to the Via della Sapienza, today’s central avenue of Corso del Rinascimento; the second stage being a major expansion towards the Piazza Navona (1496-1500) with a new, monumental façade facing the public space; and the third was the last significant expansion, carried out from 1525 to 1526 by the architect Antonio da Sangallo the Younger. Despite an intense and bustling life during the Modern Age, in the 18th century the church began to fall into ruin and was finally sold in 1878 to the order of French missionaries of Our Lady of the Sacred Heart, who reconverted it into a church and completely renovated the structure in 1881 in a project supervised by Luca Carimini. In 1936, the corrective urban redesign of Rome carried out by the fascist regime and implemented by Arnaldo Foschini mutilated the part bordering Via della Sapienza, leaving it as we see it today.

Siete Partidas

Hay un ejemplar encuadernado con NP34/1

Siete Partidas

Hay un ejemplar encuadernado con: "Las siete partidas del rey D. Alfonso el Sabio ". (XVIII/469); (XVIII/2776)

Siete Partidas

Mención de parte consta al final de la port.

Siete Partidas

Hay un ejemplar encuadernado con: Las Siete Partidas del Rey D. Alfonso el Sabio (NP34/2).

Siete Partidas

Hay un ejemplar encuadernado con el volumen facticio XVIII/2778

Siete Partidas

Hay un ejemplar encuadernado con: Las siete partidas del rey D. Alfonso el Sabio (NP34/3).

Siete Partidas

Hay un ejemplar encuadernado con: Las siete partidas del rey D. Alfonso el Sabio (NP34/3).

Liderança e satisfação dos colaboradores:um estudo de caso aplicado a organizações de economia social

Esta pesquisa investiga como o estilo de liderança adotado em três organizações de Economia Social (Instituições Sociais de Solidariedade Social) influencia o nível de satisfação dos colaboradores. A relação entre liderança e satisfação dos colaboradores tem sido estudada por muitos investigadores em diversos contextos, sobretudo na área da saúde, do ensino e em organizações com fins lucrativos, sendo escassos os estudos aplicados no sector social. Das teorias de liderança existentes, selecionou-se para investigar uma abordagem atual, pouco estudada e considerada relevante para o setor em causa: a liderança ética. A amostra abarca 97 colaboradores (90% do género feminino, 45% com o 9.º ano de escolaridade, 28% com o secundário e 27% com um curso superior, 14% desempenham funções de chefia). A idade média dos inquiridos cifra-se nos 43,8 anos (DP: 11,1) e a antiguidade média em 11,1 anos (DP: 7,7). A liderança ética foi estudada com a escala de De Hoogh e Den Hartog, (2008), abarcando três dimensões: moralidade e justiça, clarificação do papel dos colaboradores, e partilha de poder. A satisfação foi medida através da escala de Fields (2002). Controlou-se o efeito do género, da idade, das habilitações académicas, da antiguidade na organização, da antiguidade na relação com o líder, do tipo de vínculo e do exercício de funções de chefia. Os resultados sugerem a existência de diferenças significativas entre as três organizações quanto às perceções de liderança ética. Os resultados sugerem, ainda, que as perceções de liderança ética influenciam de modo positivo e significativo os níveis de satisfação das pessoas no trabalho

GÊNERO, RAÇA, DISCRIMINAÇÃO: O TOM DA COR NA DIREÇÃO DA ESCOLA PÚBLICA.

BRUNELLI, Conceição Aparecida Garcia: Gênero, raça, discriminação: o tom da cor na direção da escola pública. Mestrado em Educação. Universidade Metodista de São Paulo, São Bernardo do Campo - SP. 1 v. 244 p. 2007. Esse trabalho teve por objetivo investigar a trajetória das mulheres negras diretoras de escola pública e o processo de construção de sua identidade social, cultural, de gênero e raça. De fato, as mulheres negras em questão constroem suas identidades nadando entre águas profundas e revoltas: a das relações de gênero e a das relações raciais. A pesquisa permitiu-nos desvendar o processo seletivo pelo qual passam essas mulheres que conseguiram romper o duplo bloqueio formado pelas relações de gênero e de raça e atingiram a posição profissional de diretoras de escola pública. A questão central que norteia essa pesquisa diz respeito à trajetória de vida da mulher negra que optou pela carreira do magistério, as intercorrências encontradas ao longo de sua trajetória pessoal, de formação acadêmica e profissional, suas experiências, frustrações, expectativas, preconceitos e discriminações sofridos na caminhada até chegar ao exercício de sua atividade pública, sua ascensão social, o ingresso na carreira pública e as relações de poder que perpassam as questões de gênero e raça. Aborda ainda como essas intercorrências incidem sobre o processo de construção da identidade dessas mulheres negras e de suas relações com seus colegas brancos, homens e mulheres. A coleta de dados empíricos foi realizada através da história oral representada pela memória dessas mulheres, baseada nos depoimentos escritos e em entrevistas semi-estruturadas. Os depoimentos colhidos permitiram reunir material que foram interpretados segundo as relações de poder elaboradas por Foucault e que nos possibilitam a compreensão e uma reflexão do processo de construção das identidades individual e coletiva.

Chemically tagging the Hyades Supercluster. A homogeneous sample of F6-K4 kinematically selected northern stars

Stellar kinematic groups are kinematical coherent groups of stars that might have a common origin. These groups are dispersed throughout the Galaxy over time by the tidal effects of both Galactic rotation and disc heating, although their chemical content remains unchanged. The aim of chemical tagging is to establish that the abundances of every element in the analysis are homogeneus among the members. We study the case of the Hyades Supercluster to compile a reliable list of members (FGK stars) based on our chemical tagging analysis. For a total of 61 stars from the Hyades Supercluster, stellar atmospheric parameters (T_eff, log g, ξ, and [Fe/H]) are determined using our code called StePar, which is based on the sensitivity to the stellar atmospheric parameters of the iron EWs measured in the spectra. We derive the chemical abundances of 20 elements and find that their [X/Fe] ratios are consistent with Galactic abundance trends reported in previous studies. The chemical tagging method is applied with a carefully developed differential abundance analysis of each candidate member of the Hyades Supercluster, using a well-known member of the Hyades cluster as a reference (vB 153). We find that only 28 stars (26 dwarfs and 2 giants) are members, i.e. that 46% of our candidates are members based on the differential abundance analysis. This result confirms that the Hyades Supercluster cannot originate solely from the Hyades cluster.

Magnetic activity and differential rotation in the young Sun-like stars KIC 7985370 and KIC 7765135

Aims. We present a detailed study of the two Sun-like stars KIC 7985370 and KIC 7765135, to determine their activity level, spot distribution, and differential rotation. Both stars were previously discovered by us to be young stars and were observed by the NASA Kepler mission. Methods. The fundamental stellar parameters (vsini, spectral type, T_eff, log g, and [Fe/H]) were derived from optical spectroscopy by comparison with both standard-star and synthetic spectra. The spectra of the targets allowed us to study the chromospheric activity based on the emission in the core of hydrogen Hα and Ca ii infrared triplet (IRT) lines, which was revealed by the subtraction of inactive templates. The high-precision Kepler photometric data spanning over 229 days were then fitted with a robust spot model. Model selection and parameter estimation were performed in a Bayesian manner, using a Markov chain Monte Carlo method. Results. We find that both stars are Sun-like (of G1.5 V spectral type) and have an age of about 100–200 Myr, based on their lithium content and kinematics. Their youth is confirmed by their high level of chromospheric activity, which is comparable to that displayed by the early G-type stars in the Pleiades cluster. The Balmer decrement and flux ratio of their Ca ii-IRT lines suggest that the formation of the core of these lines occurs mainly in optically thick regions that are analogous to solar plages. The spot model applied to the Kepler photometry requires at least seven persistent spots in the case of KIC 7985370 and nine spots in the case of KIC 7765135 to provide a satisfactory fit to the data. The assumption of the longevity of the star spots, whose area is allowed to evolve with time, is at the heart of our spot-modelling approach. On both stars, the surface differential rotation is Sun-like, with the high-latitude spots rotating slower than the low-latitude ones. We found, for both stars, a rather high value of the equator-to-pole differential rotation (dΩ ≈ 0.18 rad d^-1), which disagrees with the predictions of some mean-field models of differential rotation for rapidly rotating stars. Our results agree instead with previous works on solar-type stars and other models that predict a higher latitudinal shear, increasing with equatorial angular velocity, that can vary during the magnetic cycle.

FR Cnc revisited: photometry, polarimetry and spectroscopy

This paper is part of a multiwavelength study aimed at using complementary photometric, polarimetric and spectroscopic data to achieve an understanding of the activity process in late-type stars. Here, we present the study of FR Cnc, a young, active and spotted star. We performed analysis of All Sky Automated Survey 3 (ASAS-3) data for the years 2002–08 and amended the value of the rotational period to be 0.826518 d. The amplitude of photometric variations decreased abruptly in the year 2005, while the mean brightness remained the same, which was interpreted as a quick redistribution of spots. BVR_C and I_C broad-band photometric calibration was performed for 166 stars in FR Cnc vicinity. The photometry at Terskol Observatory shows two brightening episodes, one of which occurred at the same phase as the flare of 2006 November 23. Polarimetric BVR observations indicate the probable presence of a supplementary source of polarization. We monitored FR Cnc spectroscopically during the years 2004–08. We concluded that the radial velocity changes cannot be explained by the binary nature of FR Cnc. We determined the spectral type of FR Cnc as K7V. Calculated galactic space-velocity components (U, V, W) indicate that FR Cnc belongs to the young disc population and might also belong to the IC 2391 moving group. Based on Li Iλ6707.8 measurement, we estimated the age of FR Cnc to be between 10 and 120 Myr. Doppler tomography was applied to create a starspot image of FR Cnc. We optimized the goodness of fit to the deconvolved profiles for axial inclination, equivalent width and v sin i, finding v sin  i=46.2 km s^−1 and i= 55°. We also generated a syntheticV-band light curve based on Doppler imaging that makes simultaneous use of spectroscopic and photometric data. This synthetic light curve displays the same morphology and amplitude as the observed one. The starspot distribution of FR Cnc is also of interest since it is one of the latest spectral types to have been imaged. No polar spot was detected on FR Cnc.