bluuebunny/crossref_metadata_2025_split huggingface dataset:
Design: atualidades da pesquisa em design e moda no Brasil
Authors: Moura Mônica 
Published: August 2017

O 1º Congresso Internacional de Moda e Design – CIMODE –, resultado de uma ação conjunta entre a Associação Brasileira de Estudos e Pesquisas em Moda – ABEPEM, Brasil, e da Universidade do Minho (UMinho), Portugal, marcou o ano de 2012 como um evento muito significativo para as áreas de moda e de design. O contato entre as duas instituições, somado e potencializado pelo trabalho e empenho das professoras Ana Cristina Broega e Joana Cunha, respectivamente, presidente e vice-presidente do evento, e das professoras Kathia Castilho e Dorotéia Baduy Pires, presidente e vice-presidente da ABEPEM, tornou possível a realização do Congresso, realizado na cidade de Guimarães, em Portugal, na Universidade do Minho (...)
Figurino: traje de cena: um negócio na (da) China
Authors: Viana Fausto , Muniz Rosane 
Published: August 2017

Não é de hoje que o teatro do Ocidente busca inspiração no teatro oriental. Da Índia, vieram as fortes apresentações de Kathakali e outras formas antigas de teatro e dança. Isso sem contar a febre dos filmes de Bollywood, que inspiraram obras como o filme Moulin Rouge (2001). Do Japão, os conhecidos e respeitados teatros Nô, Kabuki, Kyogen e o teatro de bonecos Bunraku, além de outras tendências mais contemporâneas, como o Butô, do qual Kazuo Ohno é o representante máximo. Do cinema japonês, é impossível não citar Akira Kurosawa (1910-1998) e obras dirigidas por ele, como Rashomon (1950), Os Sete Samurais (1954), Sonhos (1990) e Madadayo (1993) (...)
O uniforme esportivo e sua recriação televisiva
Authors: Iorio Patrícia de Miranda 
Published: August 2017

Ao comparar fotos documentais dos primeiros jogos de futebol realizados no Estado do Rio de Janeiro com produções televisivas — uma jornalística e outra ficcional — destinadas a revisitar esse período histórico, este trabalho toma como objeto de análise o uniforme esportivo para discutir a recriação televisiva. Com base nos conceitos de “bios virtual” e “telerrealidade”, do teórico da Comunicação Muniz Sodré, a investigação recai sobre a reportagem comemorativados 110 anos da primeira partida oficial de futebol no Rio, produzida pelo programa Globo Esporte, e sobre a ficção seriada Lado a lado, ambos exibidos na TV Globo.
Michel Maffesoli
Authors: Villaça Nizia 
Published: August 2017

O professor Michel Maffesoli foi meu guia nas descobertas da sensibilidade contemporâneano período de pós-doutorado, realizado em Paris V, Sorbonne. Sua sociologia do cotidiano é uma prática e uma marca da “capacidade de saber dizer sim à vida apesar de tudo” e liga-se à valorização do presente e não do “deveria ser”. O imaginário, como sublinha na entrevista,1 garante a coesão do conjunto social, sendo uma alavanca metodológica com sua solicitação do sensível. (...)
Mercado: uma análise do fashion business brasileiro
Authors: Casarim Willian Antunes 
Published: August 2017

Meu objetivo aqui é refletir sobre a maturidade do fashion business (negócio de moda) brasileiro sob a perspectiva da competitividade internacional para identificar os gaps (lacunas) da moda brasileira que têm impedido ou retardado seu avanço no cenário mundial (...)
Dijon De Moraes : “O que me deu sentido à vida foi o design”
Authors: Moura Monica 
Published: August 2017

Dijon De Moraes é um daqueles profissionais superatuantes no campo do designque ajuda a construir e a constituir o design brasileiro! É um designer no sentido mais amplo da acepção desta palavra e desta profissão: além de ser profissional ativo na área de produtos, de embalagens e de design estratégico, organizou e concebeu importantes eventos da área do design, entre eles a IV Bienal Brasileira de Design em 2012 (...)
Janelas: nada melhor que ficar amolado
Authors: Garcia Carol 
Published: August 2017

Não consigo lembrar o ano, mas deve ter sido por volta de 2004. A sala estava abarrotada e, por sorte, ela encontrava-se de costas para a porta. Nem notou que me esgueirei de mansinho, disfarçando o vexame de entrar no auditório depois de a palestra começar. Levantei o rosto cautelosamente (...)
Moda na filosofia: eu chafurdo, tu chafurdas, ele chafurda
Authors: Preciosa Rosane 
Published: August 2017

O título da dissertação é Chafurdo das cópias: histórias da Moda com bandidos e mocinhas,nobres e plebeus. O nome do autor: Humberto Piro. Aliás, um nome falso. Sublinho o falso, vocês mais adiante entenderão o porquê. O nome verdadeiro dele é Humberto Pinheiro Lopes. A defesa ocorreu em 2012, na Faculdade de Artes Visuais, na Universidade Federal de Goiás (...)
As marcas adquiriram sex appeal
Authors: Gama Maria Gabriela 
Published: August 2017

De um modo sucinto, tentamos refletir como nos relacionamos com as marcas, como estas nos aparecem como derradeiros refúgios de liberdade. Espécie de upgrads que visam colmatar espaços em branco da nossa existência estilhaçada. Falar de marcas é falar de afetos, emoções, sensações, desejos. É falar sobre relação estranha que estabelecemos com as coisas. Desenvolvemos uma ligação cada vez maior com as marcas, cultivamos, veículos intensos. Assim, a razão tecnocientífica, que tinha a pretensão de dessacralizar o real, foi explorando outras formas de sagrado, produzindo novas mitologias.
Oxo Crater on (1) Ceres: Geological History and the Role of Water-ice
Authors: Nathues A. , Platz T. , Hoffmann M. , Thangjam G. , Cloutis E. A. , Applin D. M. , Le Corre L. , Reddy V. , Mengel K. , Protopapa S. , Takir D. , Preusker F. , Schmidt B. E. , Russell C. T. 
Published: August 2017

Abstract
Dwarf planet Ceres (∅ ∼ 940 km) is the largest object in the main asteroid belt. Investigations suggest that Ceres is a thermally evolved, volatile-rich body with potential geological activity, a body that was never completely molten, but one that possibly partially differentiated into a rocky core and an ice-rich mantle, and may contain remnant internal liquid water. Thermal alteration and the infall of exogenic material contribute to producing a (dark) carbonaceous chondritic-like surface containing ammoniated phyllosilicates. Here we report imaging and spectroscopic analyses of data on the bright Oxo crater derived from the Framing Camera and the Visible and Infrared Spectrometer on board the Dawn spacecraft. We confirm that the transitional complex crater Oxo (∅ ∼ 9 km) exhibits exposed surface water-ice. We show that this water-ice-rich material is associated exclusively with two lobate deposits at pole-facing scarps, deposits that also contain carbonates and admixed phyllosilicates. Due to Oxo’s location at −4802 m below the cerean reference ellipsoid and its very young age of only 190 ka (1σ: +100 ka, −70 ka), Oxo is predestined for ongoing water-ice sublimation.
Dynamics of Massive Atmospheres
Authors: Chemke Rei , Kaspi Yohai 
Published: August 2017

Abstract
The many recently discovered terrestrial exoplanets are expected to hold a wide range of atmospheric masses. Here the dynamic-thermodynamic effects of atmospheric mass on atmospheric circulation are studied using an idealized global circulation model by systematically varying the atmospheric surface pressure. On an Earth analog planet, an increase in atmospheric mass weakens the Hadley circulation and decreases its latitudinal extent. These changes are found to be related to the reduction of the convective fluxes and net radiative cooling (due to the higher atmospheric heat capacity), which, respectively, cool the upper troposphere at mid-low latitudes and warm the troposphere at high latitudes. These together decrease the meridional temperature gradient, tropopause height and static stability. The reduction of these parameters, which play a key role in affecting the flow properties of the tropical circulation, weakens and contracts the Hadley circulation. The reduction of the meridional temperature gradient also decreases the extraction of mean potential energy to the eddy fields and the mean kinetic energy, which weakens the extratropical circulation. The decrease of the eddy kinetic energy decreases the Rhines wavelength, which is found to follow the meridional jet scale. The contraction of the jet scale in the extratropics results in multiple jets and meridional circulation cells as the atmospheric mass increases.
H2 Fluorescence in M Dwarf Systems: A Stellar Origin
Authors: Kruczek Nicholas , France Kevin , Evonosky William , Loyd R. O. Parke , Youngblood Allison , Roberge Aki , Wittenmyer Robert A. , Stocke John T. , Fleming Brian , Hoadley Keri 
Published: August 2017

Abstract
Observations of molecular hydrogen (H2) fluorescence are a potentially useful tool for measuring the H2 abundance in exoplanet atmospheres. This emission was previously observed in

dwarfs with planetary systems. However, low signal-to-noise prevented a conclusive determination of its origin. Possible sources include exoplanetary atmospheres, circumstellar gas disks, and the stellar surface. We use observations from the “Measurements of the Ultraviolet Spectral Characteristics of Low-mass Exoplanet Host Stars” Treasury Survey to study H2 fluorescence in

dwarfs. We detect fluorescence in Hubble Space Telescope spectra of 8/9 planet-hosting and 5/6 non-planet-hosting

dwarfs. The detection statistics, velocity centroids, and line widths of the emission suggest a stellar origin. We calculate H2-to-stellar-ion flux ratios to compare flux levels between stars. For stars with planets, we find an average ratio of

, using the fluxes of the brightest H2 feature and two stellar C iv lines. This is compared to

for stars without planets, showing that the planet-hosting

dwarfs do not have significant excess H2 emission. This claim is supported by the direct FUV imaging of GJ 832, where no fluorescence is observed at the expected star–planet separation. Additionally, the 3σ upper limit of 4.9 × 10−17 erg cm−2 s−1 from these observations is two orders of magnitude below the spectroscopically observed H2 flux. We constrain the location of the fluorescing H2 using 1D radiative transfer models, and find that it could reside in starspots or a ∼2500–3000

region in the lower chromosphere. The presence of this emission could complicate efforts to quantify the atmospheric abundance of H2 in exoplanets orbiting

dwarfs.
A Complete Census of Hα Emitters in NGC 6397
Authors: Pallanca Cristina , Beccari Giacomo , Ferraro Francesco R. , Pasquini Luca , Lanzoni Barbara , Mucciarelli Alessio 
Published: August 2017

Abstract
We used a data set of archival Hubble Space Telescope images obtained through the F555W, F814W, and F656N filters to perform a complete search for objects showing

emission in the globular cluster NGC 6397. As a photometric diagnostic, we used the

color excess in the

–

color–color diagram. In the analyzed field of view, we identified 53

emitters. In particular, we confirmed the optical counterpart to 20 X-ray sources (7 cataclysmic variables, 2 millisecond pulsars and 11 active binaries) and identified 33 previously unknown sources, thus significantly enlarging the population of known active binaries in this cluster. We report the main characteristics for each class of objects. Photometric estimates of the equivalent width of the

emission line were derived from the

-excess and, for the first time, compared to the spectroscopic measurements obtained from the analysis of MUSE spectra. The very good agreement between the spectroscopic and photometric measures fully confirmed the reliability of the proposed approach to measure the

emission. The search demonstrated the efficiency of this novel approach to pinpoint and measure

-emitters, thus offering a powerful tool to conduct a complete census of objects with formations and evolutions that can be strongly affected by dynamical interactions in star clusters.
Habitable Moist Atmospheres on Terrestrial Planets near the Inner Edge of the Habitable Zone around M Dwarfs
Authors: Kopparapu Ravi kumar , Wolf Eric T. , Arney Giada , Batalha Natasha E. , Haqq-Misra Jacob , Grimm Simon L. , Heng Kevin 
Published: August 2017

Abstract
Terrestrial planets in the habitable zones (HZs) of low-mass stars and cool dwarfs have received significant scrutiny recently. Transit spectroscopy of such planets with the James Webb Space Telescope (JWST) represents our best shot at obtaining the spectrum of a habitable planet within the next decade. As these planets are likely tidally locked, improved 3D numerical simulations of such planetary atmospheres are needed to guide target selection. Here we use a 3D climate system model, updated with new water-vapor absorption coefficients derived from the HITRAN 2012 database, to study ocean-covered planets at the inner edge of the HZ around late M to mid-K stars (

). Our results indicate that these updated water-vapor coefficients result in significant warming compared to previous studies, so the inner HZ around M dwarfs is not as close as suggested by earlier work. Assuming synchronously rotating Earth-sized and Earth-mass planets with background 1 bar

atmospheres, we find that planets at the inner HZ of stars with

undergo the classical “moist greenhouse” (

mixing ratio

in the stratosphere) at significantly lower surface temperature (∼280 K) in our 3D model compared with 1D climate models (∼340 K). This implies that some planets around low-mass stars can simultaneously undergo water loss and remain habitable. However, for stars with

, planets at the inner HZ may directly transition to a runaway state, while bypassing the moist greenhouse water loss entirely. We analyze transmission spectra of planets in a moist greenhouse regime and find that there are several prominent

features, including a broad feature between 5 and 8 μm, within JWST MIRI instrument range. Thus, relying only on standard Earth-analog spectra with 24 hr rotation period around M dwarfs for habitability studies will miss the strong

features that one would expect to see on synchronously rotating planets around M dwarf stars, with JWST.
Optical Properties of Non-stoichiometric Amorphous Silicates with Application to Circumstellar Dust Extinction
Authors: Tamanai Akemi , Pucci Annemarie , Dohmen Ralf , Gail Hans-Peter 
Published: August 2017

Abstract
We determine the optical constants of non-stoichiometric amorphous magnesium-iron silicates and demonstrate that they can well reproduce the observed mid-infrared emission spectra of evolved stars. Stoichiometric and non-stoichiometric amorphous magnesium-iron silicate films are fabricated by pulsed laser deposition. Transmittance and ellipsometry measurements are performed in the wavelength range between 2 and 200 μm and 1.7 and 33 μm, respectively. Optical constants are derived from transmittance and ellipsometric Ψ and Δ spectra by means of oscillator models. These newly obtained optical constants are applied in radiative transfer models for examining reproducibility of the observed spectral features of circumstellar dust shells around supergiants. The spectra of four selected supergiants are dominated by amorphous silicate dust emission in the wavelength range between 9 and

. To obtain a good fit to the observed spectra, we take into account amorphous corundum and metallic iron particles as additional dust components to the model calculations to rationalize the dust emission at

. For each of the objects, a set of model parameters (dust mass and condensation temperature) is derived by an automated optimization procedure that reproduces the observation well. Consequently, our model spectra using new optical data reveal that the silicate bands at ∼10 and

depend on the magnesium and iron ratio in the silicate system, and that a good fit requires a significant iron content of the amorphous silicate dust component to reproduce the observed peak positions and shape of the silicate bands.
Strongly Misaligned Triple System in SR 24 Revealed by ALMA
Authors: Fernández-López M. , Zapata L. A. , Gabbasov R. 
Published: August 2017

Abstract
We report the detection of the 1.3 mm continuum and the molecular emission of the disks of the young triple system SR24 by analyzing ALMA (The Atacama Large Millimeter/Submillimter Array) subarcsecond archival observations. We estimate the mass of the disks (0.025 M
☉ and 4 × 10−5
M
⊕ for SR24S and SR24N, respectively) and the dynamical mass of the protostars (1.5 M
☉ and 1.1 M
☉). A kinematic model of the SR24S disk to fit its C18O (2-1) emission allows us to develop an observational method to determine the tilt of a rotating and accreting disk. We derive the size, inclination, position angle, and sense of rotation of each disk, finding that they are strongly misaligned (

) and possibly rotate in opposite directions as seen from Earth, in projection. We compare the ALMA observations with 12CO SMA archival observations, which are more sensitive to extended structures. We find three extended structures and estimate their masses: a molecular bridge joining the disks of the system, a molecular gas reservoir associated with SR24N, and a gas streamer associated with SR24S. Finally, we discuss the possible origin of the misaligned SR24 system, concluding that a closer inspection of the northern gas reservoir is needed to better understand it.
The Infrared Medium-deep Survey. III. Survey of Luminous Quasars at 4.7 ≤ z ≤ 5.4*
Authors: Jeon Yiseul , Im Myungshin , Kim Dohyeong , Kim Yongjung , Jun Hyunsung David , Pak Soojong , Taak Yoon Chan , Baek Giseon , Choi Changsu , Choi Nahyun , Hong Jueun , Hyun Minhee , Ji Tae-Geun , Karouzos Marios , Kim Duho , Kim Jae-Woo , Kim Ji Hoon , Kim Minjin , Kim Sanghyuk , Lee Hye-In , Lee Seong-Kook , Park Won-Kee , Park Woojin , Yoon Yongmin 
Published: August 2017

Abstract
We present the first results of our survey for high-redshift quasars at

. The search for quasars in this redshift range has been known to be challenging due to the limitations of the filter sets used in previous studies. We conducted a quasar survey for two specific redshift ranges, 4.60 ≤ z ≤ 5.40 and 5.50 ≤ z ≤ 6.05, using multi-wavelength data that include observations made with custom-designed filters, is and iz. Using these filters and a new selection technique, we were able to reduce the fraction of interlopers. Through optical spectroscopy, we confirmed six quasars at 4.7 ≤ z ≤ 5.4 with

that recently were discovered independently by another group. We estimated black hole masses and Eddington ratios of four of these quasars from optical and near-infrared spectra, and found that these quasars are undergoing nearly Eddington-limited accretion that is consistent with the rapid growth of supermassive black holes in luminous quasars at z ∼ 5.
Le déclin des cartels dans l’économie de la RFA
Authors: Schröter Harm G. , Joly Hervé , Dupré Michèle 
Published: August 2017

Jusqu’en 1945, l’opinion s’était répandue en Allemagne, parmi les industriels, les organisations patronales, les syndicats, les gouvernements, et aussi parmi la majorité des économistes, que les cartels permettraient de remettre en partie de l’ordre dans les tendances chaotiques du capitalisme. Les mentalités étaient fortement orientées en faveur de la cartellisation. Mais l’interdiction américaine des cartels, l’engagement d’économistes allemands et le développement économique exceptionnel des années 1950 et 1960 ont ensuite inversé, sur la base d’une économie structurellement transformée dans un sens défavorable aux cartels, cette appréciation positive. L’évolution s’est cependant, comme tout changement de mentalité, étalée sur de nombreuses années. Elle est même en partie remise en cause depuis les années 1980, en particulier au niveau de la Communauté Européenne : les cartels sont maintenant perçus, dans des circonstances particulières, comme une possibilité de surmonter des crises.
L’entreprise formatrice entre tradition et contestation
Authors: Lattard Alain 
Published: August 2017

Le système d’apprentissage n’est pas seulement « dual » par rapport aux lieux d’apprentissage (entreprise / école), il l’est aussi par rapport aux modes de régulation de l’offre (marché libre pour la quantité / standardisation pour la qualité) et au partage du pouvoir (patronat / syndicat). C’est la centralité de l’entreprise qui donne sa cohérence au dispositif, mais la participation syndicale qui lui donne sa légitimité. La genèse du système dual remonte au tournant du siècle, lorsque l’artisanat obtient une représentation corporative et le monopole de l’apprentissage. Ce monopole est bientôt contesté par l’industrie, au nom des besoins modernes de qualification et par le syndicalisme, au nom de la démocratie économique. La synthèse de ces trois apports successifs est tardive. Si l’industrie intègre le système au milieu des années 1930, le syndicalisme en reste exclu jusqu’à la fin des années 1960. Aujourd’hui, le système doit faire face à l’attrait pour les études supérieures et aux exigences de réduction des coûts qui conduisent au désengagement graduel des entreprises.
Éditorial. Face aux risques écologiques, des mobilisations variables
Authors: Giblin Béatrice 
Published: August 2017

L’écologie politique n’est plus le domaine réservé des partis écologistes. Désormais, les risques écologiques (réchauffement climatique, pollution de l’air, pesticides, etc.) se sont imposés à tous dans les pays riches comme dans les pays émergents. Mais ce n’est pas pour autant que les comportements de tout un chacun et les politiques mises en œuvre par les dirigeants les prennent sérieusement en compte. Le chemin est long entre la prise de conscience des risques et la mise en œuvre des actes pour les limiter. Seules les catastrophes écologiques, mais aussi les atteintes aux paysages et les conséquences négatives sur la santé des individus de certaines pratiques liées à une économie productiviste suscitent la mobilisation de la population concernée et contraignent les responsables politiques à intervenir.
De Notre-Dame-des-Landes à Bure, la folle décennie des « zones à défendre » (2008-2017)
Authors: Subra Philippe 
Published: August 2017

Les années 2008-2017 ont vu l’apparition en France de « zones à défendre », une forme de lutte nouvelle qui renouvelle profondément la scène contestataire, par ses modalités (l’occupation permanente des sites des projets contestés pour empêcher le démarrage des chantiers) et par ses acteurs (des militants altermondialistes). La résistance physique à l’expulsion, une bonne utilisation des réseaux sociaux et des médias, l’action de nombreux comités de soutien modifient les rapports de forces entre porteurs des projets et opposants et posent des problèmes inédits à l’État : comment réussir à expulser les zadistes ? Quelle place pour la concertation ? Le référendum local est-il la solution ?
Comparer la réussite des conflits environnementaux en Allemagne et en France : une approche géopolitique
Authors: Meyer Teva 
Published: August 2017

Que l’on considère le poids des associations de protection de la nature, la réussite électorale des partis écologistes ou les politiques publiques engagées, les mouvements environnementalistes allemands apparaissent en avance sur leurs homologues français. Loin de toute approche culturaliste, ce succès relatif est la conséquence de rapports de forces, de stratégies d’acteurs ainsi que de représentations géopolitiques et s’appuie sur des structures fédérales plus favorables outre-Rhin. Après avoir synthétisé les débats scientifiques sur les raisons de cet écart franco-allemand, cet article propose d’analyser une décision emblématique de l’environnementalisme outre-Rhin : l’accélération de la sortie du nucléaire en 2011. Celle-ci permet de montrer que, loin d’être uniquement portée par un mouvement écologiste, la réussite de l’environnementalisme allemand est le produit de coalitions mêlant des acteurs aux motivations divergentes, mais aux intérêts communs.