Unraveling the Dust Formation Process in R Dor

Using both dynamical and chemical modelling, we derive an accurate abundance profile for the molecule SiO in the stellar wind of R Dor, an O-rich AGB star. SiO plays a key role in the dust formation process in O-rich AGB stars. This method will be applied to additional molecules, with the aim to achieve a detailed overview of the molecular abundance pattern in the wind of R Dor.

Chromatic Aberration

Chromatic Aberration is a film installation which explores the early technologies of colour filmmaking drawn from the archives of George Eastman House, Rochester, New York. Featuring vibrant close-ups of eyes from fledgling archival experiments in colour film, Chromatic Aberration turns the cinematic lens in on itself: from the prosthetic recording eye of the camera, to an evocation of the abstract inner screen of one's eyelids. Early 1920s colour film footage - mainly tests shots featuring members of George Eastman's family as well as Hollywood stars of the time - is shot in such a way so as to reveal the inherent chromatic fringing, distortion and misalignment. Using specialist equipment at the BFI National Archive, London, the footage is reworked through the use of extreme close-up and magnification, honing in on the eyes. The installation evokes an imagined abstract colour world, a flickering eyelid trapped in a mechanical peephole. Exhibitions: Solo exhibition as film installation at Tyneside Cinema (Newcastle, Oct-Nov 2014); Solo exhibition at George Eastman Museum (Rochester, New York, Jan-April 2015), including a second work on display. Film festivals nominations for competitions: Winner of Best Vanguard Film Competition in Lima Independiente International Film Festival (Peru). Nominations: Filmadrid festival (Spain); Curtas Vila do Conde film festival (Portugal); Festival du Nouveau Cinema (Canada); Jihlava International Documentary Film Festival (Czech Republic ); International Film Festival Bratislava (Slovenia). Additional screenings at International Rotterdam Film Festival (Netherlands); European Media Art Festival (Germany); BFI London Film Festival (UK); Mini-retrospective screening at DIM CINEMA, The Cinematheque (Vancouver May 2015). Reviews and interviews in Artforum, The Wire Magazine, After Image, Studio International. Public lectures: with Prof. Sarah Street at Tyneside Cinema (Nov 2014); Royal Academy visiting public lecture (Nov 2014); ‘The Laughter of Things’ symposium, International Film Festival Rotterdam and Piet Zwart Institute (Jan 2015); George Eastman Museum and Rochester University (April 2015). Acquired by the George Eastman Museum for their collection.

Modos r de oscilação em estrelas de neutrões

Tese dout., Física - Astrofísica, Universidade do Algarve, 2007

Beach quality assessment and management in the Sotavento (Eastern) Algarve, Portugal

The purpose of this study on beach quality assessment and management was to evaluate the quality of five beaches in the Algarve Sotavento region of Portugal and to identify beach users’ preferences and priorities regarding their visit to a beach. The Algarve is one of the country’s most internationally known regions and it is generally perceived as a major tourist destination. Because of the increasing level of tourists, there is a specific need to address beach quality, as overcrowding can result in excessive litter, reduce water quality and consequently reduce the socio-economic value of the area. The main methodology for the evaluation of the beach quality in this pilot project was the Bathing Area Registration and Evaluation framework (BARE), which recognizes five beach types (rural, remote, resort, urban and village) through five main priority issues of concern to beach users (water quality, scenery, litter, safety, facilities) and evaluates the beach quality, ranging from one (low) to five (high) stars. After overall bathing area classification, Quarteira-Vilamoura, Ilha do Farol, Ilha Deserta and Ilha da Armona received three-star rating and Quinta do Lago site obtained a one-star rating. The quantitative research data on beach users’ preferences and priorities was obtained through administration of 50 questionnaires per beach and showed that beach users at all sites expressed the need for improved cleanliness, safety and facilities on the beach. The BARE framework, together with the questionnaire surveys, allowed the identification of management priorities required to improve the quality of individual beaches and therefore increase income from tourism.

Crieff Hydro Hotel: the experience economy and the guest perspective

The purpose of this report is to do a presentation of the hotel where I will be working, characterising the reception department and all the activities that I developed during this placement. On this placement at the CHH (Crieff Hydro Hotel) – family 4 stars resort, my goal is to have an experience in hospitality, in special in reception. This placement is carried out from my Master degree in Direcção e Gestão Hoteleira (Commercial branch) at the University of the Algarve – Campus Penha. For this report it was also intended to do an analysis of the guest experience in hospitality and for that it was necessary to do a literature review adequate for my area of work in the hotel giving importance to the guest experience in the hospitality. For my analysis regarding the guest experience in hospitality, I used data collected from the surveys answered by the guests that stayed with us in the hotel. To analyse the data it was necessary to do a categorial analysis technique. After this year of placement in the hotel and after this analysis, as results I have the opportunity to continue my work in the hotel and also the possibility of a better position in a near future. Last but not least, this report demonstrates my work path and also helps to have a better understanding of the satisfaction perceived by the guest in order to give us tools to improve it. From what we can see, the guests’ satisfaction is highly rated on both surveys.

Guest reputation indexes to analyze hotel’s online reputation using data extracted from OTAs

Nowadays many travelers use online travel agency (OTAs) to book flights, hotel rooms, rent-a-cars, cruises or entire vacation packages. Usually OTAs allow their users to give scores and to write reviews about what was used. Each OTA defines the terms and conditions for guest rating or review score and hoteliers are giving increasing importance to the scores and reviews their guests do in OTAs. This paper proposes two guest reputation index to help hoteliers to monitorize their presence in OTAs. The Aggregated Guest Reputation Index (AGRI), which shows the positioning of a hotel in different OTAs and it is calculated from the scores obtained by the hotels in those OTAs. Another one, the Semantic Guest Reputation Index (SGRI), which incorporates the social reputation of a hotel and that can be visualized through the development of word clouds or tag clouds. Examples of usage of these indexes are given with data extracted from 5-stars hotels in the Algarve, south region of Portugal, that are available on Booking and Expedia.

Vom Trümmerfilm zur Traumfabrik : die "Junge Film-Union". Eine Fallstudie zur westdeutschen Filmproduktion

Die Trümmer des deutschen Reiches waren 1945 auch die Trümmer des deutschen Films. Der Neuaufbau der deutschen Filmwirtschaft, der unter der Ägide der Alliierten begann, eröffnete trotz zahlloser Schwierigkeiten neue Chancen, nicht zuletzt regional: auch Niedersachsen wurde "Filmland". Die "Junge Film-Union", 1947 lizensiert, wurde bald zur größten niedersächsischen Filmproduktionsfirma. Waren die ersten zeitnahen Filme - auch "Trümmerfilme" genannt - noch in mancher Hinsicht improvisiert, so professionalisierte sich die Produktion zusehends. Es wurden eigene Ateliers gebaut, in dem Heideort Bendestorf entstand in kurzer Zeit eine Filmindustrie. Und auch die Filmstoffe wandelten sich, ebenso die Besetzung der Hauptrollen: der "zeitlose" Unterhaltungsfilm wurde selbstverständlich, ein neuer Kult mit alten Stars verdrängte den Nachwuchs. Neben vielen Mißerfolgen der "Jungen Film-Union" wurde schließlich "Die Sünderin" zu einem (Skandal-)Erfolg, der Marika-Rökk-Film "Die Csardas-Fürstin" ein echter Publikumsrenner. Der spektakuläre Neuaufbau dieser Filmproduktion, die wechselvolle Entwicklung, die im Konkurs 1952 ein jähes Ende fand, werfen Fragen auf, denen in dieser Arbeit auf der Basis neuen Quellenmaterials nachgegangen wird. Welche politischen, ökonomischen und kulturellen Einflüsse waren es, die für die "Junge Film-Union" bestimmend wurden. Welche Rolle spielte die britische Filmpolitik? Welche Bedeutung hatte die Währungsreform, wie wirkten sich die Bundesbürgschaften aus? Welche filmischen Traditionen wurden aufgegriffen, und wie spiegelt sich die außerfilmische Realität in den Produktionen? Die Ergebnisse der Untersuchung werfen dabei auch ein Licht auf den Neuaufbau der westdeutschen Filmwirtschaft insgesamt.

Pope as media star: a long career full of reinvention

On the whole, a man who is elected as Pope is well on in years. Some, despite this, have managed to reign for a long time, Leo XIII for instance who came to the throne when he was already seventy in 1878, reigned for twenty five years. Wojtyla was elected when he was only fifty eight, in 1978. In the last century or so, the papacy has become visible worldwide through the mass media. On his accession, Wojtyla was presented as a man's man, a sportsman - according to Professor Eamon Duffy of Cambridge University - as a Bishop with balls. Like other media stars who have stayed the test of time, e.g. Madonna, David Bowie, it seems that he has been able to reinvent his media image to some extent; from the active sportsman to the benevolent grandfather to the ailing figure we see today. He has taken on the aspect of a media star, a world traveller, a spiritual leader, a politician, a mediator and a peace leader. He has been described as the most-photographed person on the planet. This paper will attempt to trace these changes and to ascertain, using Vatican and media sources to discover how much of this continual change is driven by the personality of John Paul himself and how much is a deliberate policy on the part of the Vatican.

The influence of salinity and sea star wasting syndrome on sea star species composition and distribution in Nootka Sound, British Columbia

Senior thesis written for Oceanography 445

Prática de ensino supervisionado no 1.º e 2.º ciclo do ensino básico: de que modo o recurso às tecnologias de comunicação e de informação altera as conceções alternativas acerca dos astros em alunos do 1.ª ciclo do ensino básico

Relatório apresentado à Escola Superior de Educação de Lisboa para obtenção do grau de mestre em Ensino do 1.º e do 2.º Ciclo do Ensino Básico

Hotel industry: An answer to the emerging trends on the global demand side of tourism

This dissertation studies essentially how Millennials are changing the hotel industry, in the sense that new trends are emerging with this generation and hotels need to respond accordingly, in order to survive within their competitive industry. Emphasis is also given to Asian travellers, as the enlargement of these countries’ middle class populations is predicted, therefore making Asian travellers a valuable target for the hotel industry. To successfully target this segment, hoteliers need also to consider the cultural differences and aspirations that come together with the Asian travellers, and appropriately adapt their offer to them. I will then redirect this study to the city of Lisbon, the Portuguese capital, to analyse if Lisbon’s four and five-star hotel managers are aware of the new market trends, and to understand how they are changing their hotels in order to make them more attractive to Millennials and Asian travellers. Using a sample of 12 hotels (four and five-stars ratings), I have concluded that, although there is a notable undergoing process of adaptation to these guests, there is a long way ahead in order for Lisbon’s hotels to entirely please and retain millennial guests.

Heidegger's tragic Greeks : the relation between presence and deinon

Martin Heidegger's interpretation of the ancients was born out of something like a crisis in the interpretation of the Greeks, which can be characterized as nothing other than the realization of the idea that the Greek philosophers put a serious question mark over existence. This idea, which had its germination in Prussia with Jakob Burckhart and his teacher, but first came to be seriously cultivated in the Philosophy of Friedrich Nietzsche, was the first in depth investigation into whether the Greeks, on the one hand, questioned existence or, on the other hand, put a question mark over existence. To question existence is rather innocuous, since it amounts to little more, in the end, than a child looking up at the stars and asking what it all means. To put a question mark over existence, however, is another business entirely. For the Greeks, as the life work of Martin Heidegger amply demonstrates, the nature of Greek thinking and the objects towards which it is directed follows so absolutely from the tragic view of the human person that, in a certain sense, philosophy is Greek and could only have developed in Greece. Perhaps stating it a little less categorically, philosophy could have developed elsewhere at least to the extent that something like they way the Greeks understood life was at the forefront: presence, in other words. This thesis deals with the problem ofHeidegger's relation to the Greeks, specifically in terms of his understanding of the Greeks and presence. It is the position of this dissertation that the Greek notion of presence is, as Heidegger understands it, the homeliness of the hearth that radiates through all the things that humans concern themselves with. This is thought by Heidegger, as the Greeks did, specifically in contrast with the uncanninesslunhomeliness of the hqrnan apart from his or her concern with things. Therefore, the thesis is an attempt at exposing the relation between presence and the unhomely by situating it withing Greek existence and the meaning of the Greek Philosopher. In order to support this position, the thesis has been divided into five parts. The first two chapters deal with Heidegger's explanation of the relation between Greek notion of physics (Phusis), metaphysics (specifically in relation to an analysis of time and motion in Greek thought), and what Heidegger calls the fundamental attunement of Dasein (boredom). More exactly, it deals with these issues only so far as they allow us to bring out something like the notion of 'presence' in relation to things and homelessness or restlessness in relation to the human being. The rationale for these two chapters in relation to the central problem of the paper is that in Heidegger's elucidation of physics and metaphysics, he conducts his analysis in such a way that he explicitly uncovers that dimension of human existence that he calls the fundamental attunement of Dasein. This fundamental attunement is, in tum, similar to what the Greeks understood as the deinon, the uncanninesslunhomeliness of the human. The third and fourth chapters take as their explicit themes the problem of the Greek understanding of the assertion and the ways in which the person can comport himlherself toward things, two issues which are not separable. The rationale for these two chapters in relation to the central theme of the paper is that Heidegger's analysis of these two areas in Greek thought brings out precisely why the philosopher and the philosophical way of life is the highest mode of existence for the Greeks and how this is thought specifically in tenns of the uncanniness of humans. The final cijapter gives a complete elucidation of presence as the homeliness of the hearth and shows specifically how this is thought of in contradistinction to the uncanny/unhomely for the Greeks. 1I1 This last chapter also explains Martin Heidegger's reaction to the Greek's interpretation of the highest mode of existence, and what he posited as a counter-thought. The essay as a whole is an attempt to fully concertize an important dimension of Heidegger' s understanding of the Greeks, that is, the relation between presence and the deinon or Greek notion ofunhomely, which, to my la)owledge, has not been offered anywhere in commentaries on Heidegger.

Buying Britney : pop culture icons to cultural brands

This thesis demonstrates that mUSIC stars who attain cultural icon status heavily contribute to the fashion styles of the time. Where as style and music have always had a connection, icons such as Britney Spears are now dictating popular style so much so that music artists are becoming full-fledged fashion designers. While much analysis is devoted to Britney Spears, her largest contributions do not lie in the rise of teenage sexuality, but in establishing music artists as vehicles of consumption. The artists' signature has now become a brand and ~ term "signabrand" has been created to define such a trend. To understand such a shift, a review of past literature devoted to fashion and music, largely consisting of subculture theory is examined, followed by a combination of content analysis, political economy, fashion and postmodem theory to address how music stars attain icon status and guide style.

Étude de l’étoile Wolf-Rayet variable WR 46 dans l’ultraviolet lointain et les rayons X

L’étoile Wolf-Rayet WR 46 est connue pour sa variabilité complexe sur des échelles de temps relativement courtes de quelques heures et sur des échelles de temps plus longues de plusieurs mois. Des décalages périodiques mais intermittents en vitesse radiale ont déjà été observés dans ses raies d’émission optiques. Plusieurs périodes photométriques ont aussi été mesurées dans le passé. Des pulsations non-radiales, une modulation liée à la rotation rapide, ou encore la présence d’un compagnon de faible masse dont la présence reste à confirmer ont été proposées pour expliquer le comportement de l’étoile sur des échelles de temps de quelques heures. Dans un effort pour dévoiler sa vraie nature, nous avons observé WR 46 avec le satellite FUSE sur plusieurs cycles de variabilité à court terme. Nous avons trouvé des variations sur une échelle de temps d’environ 7,5 heures dans le continu ultraviolet lointain, dans l’aile bleue de la composante d’absorption du profil P Cygni du doublet de O vi 1032, 1038, ainsi que dans la composante d’absorption du profil P Cygni de S vi 933, 944. Nous avons également récupéré des données archivées de cette étoile obtenues avec le satellite XMM-Newton. La courbe de lumière en rayons X montre des variations sur une échelle de temps similaire aux courbes de lumière du continu ultraviolet et ultraviolet lointain, et le spectre rayons X de WR 46 est très mou avec un pic d’émission à des énergies plus faibles que 1 keV. Nous discutons des différentes contraintes sur la nature de la variabilité de cette étoile que ces nouvelles observations aident à poser. Parmi les scénarios suggérés, nous concluons que celui des pulsations non-radiales est le plus probable, bien que nous soyons encore loin d’une compréhension détaillée de WR 46.

Étude spectroscopique d'étoiles naines blanches riches en hélium de type DB et DBA

De nouveaux modèles d'atmosphère sont présentés, incluant les profils de raie d'hélium neutre améliorés de Beauchamp (1995) et le formalisme de probabilité d'occupation pour ce même atome. Ces modèles sont utilisés pour calculer une grille de spectres synthétiques correspondant à des atmosphères riches en hélium et contenant des traces d'hydrogène. Cette grille est utilisée pour déterminer les paramètres atmosphériques principaux des étoiles de notre échantillon, soient la température effective, la gravité de surface et l'abondance d'hydrogène. Notre échantillon contient des spectres visibles de haut rapport signal-sur-bruit pour 102 naines blanches riches en hélium, dont 29 ont été observés au cours de ce projet, ce qui en fait le plus grand échantillon de spectres de qualité de naines blanches riches en hélium. Des spectres synthétiques ont été calculés en utilisant différentes valeurs du paramètre α de la théorie de la longueur de mélange dans le but de calibrer empiriquement la valeur de ce paramètre pour les DB. Afin d'améliorer la précision sur les paramètres atmosphériques de quelques étoiles, nous avons utilisé des spectres couvrant la raie Hα pour mieux déterminer l'abondance d'hydrogène. Finalement, nous avons calculé la distribution de masse de notre échantillon et la fonction de luminosité des DB. La distribution de masse montre une coupure à 0.5 fois la masse solaire qui est prédite par les modèles d'évolution stellaire et dévoile une masse moyenne significativement plus élevée pour les étoiles de type DBA. La masse moyenne de l'ensemble des DB et DBA est très proche de celle des DA. La fonction de luminosité nous permet de calculer que le rapport du nombre de DB sur le nombre de DA vaut environ 25%.