Line-profile tomography of exoplanet transits - II. A gas-giant planet transiting a rapidly rotating A5 star

Most of our knowledge of extrasolar planets rests on precise radial-velocity measurements, either for direct detection or for confirmation of the planetary origin of photometric transit signals. This has limited our exploration of the parameter space of exoplanet hosts to solar- and later-type, sharp-lined stars. Here we extend the realm of stars with known planetary companions to include hot, fast-rotating stars. Planet-like transits have previously been reported in the light curve obtained by the SuperWASP survey of the A5 star HD15082 (WASP-33 V = 8.3, v sini = 86 km s-1). Here we report further photometry and time-series spectroscopy through three separate transits, which we use to confirm the existence of a gas-giant planet with an orbital period of 1.22d in orbit around HD15082. From the photometry and the properties of the planet signal travelling through the spectral line profiles during the transit, we directly derive the size of the planet, the inclination and obliquity of its orbital plane and its retrograde orbital motion relative to the spin of the star. This kind of analysis opens the way to studying the formation of planets around a whole new class of young, early-type stars, hence under different physical conditions and generally in an earlier stage of formation than in sharp-lined late-type stars. The reflex orbital motion of the star caused by the transiting planet is small, yielding an upper mass limit of 4.1MJupiter on the planet. We also find evidence of a third body of substellar mass in the system, which may explain the unusual orbit of the transiting planet. In HD 15082, the stellar line profiles also show evidence of non-radial pulsations, clearly distinct from the planetary transit signal. This raises the intriguing possibility that tides raised by the close-in planet may excite or amplify the pulsations in such stars.

A survey for planetary transits in the field of NGC 7789

We present results from 30 nights of observations of the open cluster NGC 7789 with the Wide Field Camera on the Isaac Newton Telescope, La Palma. From ~900 epochs, we obtained light curves and Sloan r'-i' colours for ~33000 stars, with ~2400 stars having better than 1 per cent precision. We expected to detect ~2 transiting hot Jupiter planets if 1 per cent of stars host such a companion and a typical hot Jupiter radius is ~1.2R_J. We find 24 transit candidates, 14 of which we can assign a period. We rule out the transiting planet model for 21 of these candidates using various robust arguments. For two candidates, we are unable to decide on their nature, although it seems most likely that they are eclipsing binaries as well. We have one candidate exhibiting a single eclipse, for which we derive a radius of 1.81+0.09-0.00R_J. Three candidates remain that require follow-up observations in order to determine their nature.

Butor et le livre-installation: montage de textes, œuvre plurielle, transits entre univers culturels

La complétude des Œuvres complètes de Butor est problématique, car elle ne prend pas en compte les collaborations de toutes sortes et les œuvres inscrites sur d’autres supports que du papier. Pour avoir une véritable idée de cette complétude, il faudrait donc imaginer une installation qui réunirait à la fois, entre autres, les codex habituels de Butor, les livres d’artistes, les œuvres numériques. On se rendrait compte que cette installation est fondée sur des passages de frontières entre les genres artistiques, l’assemblage et le collage permettant de passer des frontières entre univers culturels différents.

CHEOPS: a space telescope for ultra-high precision photometry of exoplanet transits

The CHaracterising ExOPlanet Satellite (CHEOPS) is a joint ESA-Switzerland space mission (expected to launch in 2017) dedicated to search for exoplanet transits by means of ultra-high precision photometry. CHEOPS will provide accurate radii for planets down to Earth size. Targets will mainly come from radial velocity surveys. The CHEOPS instrument is an optical space telescope of 30 cm clear aperture with a single focal plane CCD detector. The tube assembly is passively cooled and thermally controlled to support high precision, low noise photometry. The telescope feeds a re-imaging optic, which supports the straylight suppression concept to achieve the required Signal to Noise. © (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.

Tables to facilitate the reduction of transits, arranged for use at the Royal observatory, Greenwich.

Mode of access: Internet.

An asymptotic analysis for the coupled dispersion characteristics of a structural acoustic waveguide

Analytical expressions are derived, using asymptotics, for the fluid-structure coupled wavenumbers in a one-dimensional (1-D) structural acoustic waveguide. The coupled dispersion equation of the system is rewritten in the form of the uncoupled dispersion equation with an added term due to the fluid-structure coupling. As a result of this coupling, the prior uncoupled structural and acoustic wavenumbers, now become coupled structural and acoustic wavenumbers. A fluid-loading parameter e, defined as the ratio of mass of fluid to mass of the structure per unit area, is introduced which when set to zero yields the uncoupled dispersion equation. The coupled wavenumber is then expressed in terms of an asymptotic series in e. Analytical expressions are found as e is varied from small to large values. Different asymptotic expansions are used for different frequency ranges with continuous transitions occurring between them. This systematic derivation helps to continuously track the wavenumber solutions as the fluid-loading parameter is varied from small to large values. Though the asymptotic expansion used is limited to the first-order correction factor, the results are close to the numerical results. A general trend is that a given wavenumber branch transits from a rigid-walled solution to a pressure-release solution with increasing E. Also, it is found that at any frequency where two wavenumbers intersect in the uncoupled analysis, there is no more an-intersection in the coupled case, but a gap is created at that frequency. (c) 2007 Elsevier Ltd. All rights reserved.

Asymptotic analysis for the coupled wavenumbers in an infinite fluid-filled flexible cylindrical shell: The axisymmetric mode

The coupled wavenumbers of a fluid-filled flexible cylindrical shell vibrating in the axisymmetric mode are studied. The coupled dispersion equation of the system is rewritten in the form of the uncoupled dispersion equation of the structure and the acoustic fluid, with an added fluid-loading term involving a parameter e due to the coupling. Using the smallness of Poisson's ratio (v), a double-asymptotic expansion involving e and v 2 is substituted in this equation. Analytical expressions are derived for the coupled wavenumbers (for large and small values of E). Different asymptotic expansions are used for different frequency ranges with continuous transitions occurring between them. The wavenumber solutions are continuously tracked as e varies from small to large values. A general trend observed is that a given wavenumber branch transits from a rigidwalled solution to a pressure-release solution with increasing E. Also, it is found that at any frequency where two wavenumbers intersect in the uncoupled analysis, there is no more an intersection in the coupled case, but a gap is created at that frequency. Only the axisymmetric mode is considered. However, the method can be extended to the higher order modes.

On the mechanism and the length scales involved in the ductile fracture of a bulk metallic glass

Some bulk metallic glasses (BMGs) exhibit high crack initiation toughness due to shear band mediated plastic flow at the crack tip and yet do not display additional resistance to crack growth due to the lack of a microstructure. Thus, at crack initiation, the fracture behavior of BMGs transits from that of ductile alloys to that of brittle ceramics. In this paper, we attempt to understand the physics behind the characteristic length from the notch root at which this transition occurs, through testing of four-point bend specimens made of a nominally ductile Zr-based BMG in three different structural states. In the as-cast state, both symmetric (mode I) and asymmetric (mixed mode) bend specimens are tested. The process of shear band mediated plastic flow followed by crack initiation at the notch root was monitored through in situ imaging. Results show that stable crack growth occurs inside a dominant shear band through a distance of, similar to 60 mu m, irrespective of the structural state and mode mixity, before attaining criticality. Detailed finite element simulations show that this length corresponds to the distance from the notch root over which a positive hydrostatic stress gradient prevails. The mean ridge heights on fractured surfaces are found to correlate with the toughness of the BMG. The Argon and Salama model, which is based on the meniscus instability phenomenon at the notch root, is modified to explain the experimentally observed physics of fracture in ductile BMGs. (C) 2012 Acta Materialia Inc. Published by Elsevier Ltd. All rights reserved.

Acoustic response of vortex breakdown modes in a coaxial isothermal unconfined swirling jet

The present experimental work is concerned with the study of amplitude dependent acoustic response of an isothermal coaxial swirling jet. The excitation amplitude is increased in five distinct steps at the burner's Helmholtz resonator mode (i.e., 100 Hz). Two flow states are compared, namely, sub-critical and super-critical vortex breakdown (VB) that occur before and after the critical conical sheet breakdown, respectively. The geometric swirl number is varied in the range 2.14-4.03. Under the influence of external pulsing, global response characteristics are studied based on the topological changes observed in time-averaged 2D flow field. These are obtained from high resolution 2D PIV (particle image velocimetry) in the longitudinal-mid plane. PIV results also illustrate the changes in the normalized vortex core coordinates (r(vcc)/(r(vcc))(0) (Hz), y(vcc)/(y(vcc))(0) (Hz)) of internal recirculation zone (IRZ). A strong forced response is observed at 100 Hz (excitation frequency) in the convectively unstable region which get amplified based on the magnitude of external forcing. The radial extent of this forced response region at a given excitation amplitude is represented by the acoustic response region (b). The topological placement of the responsive convectively unstable region is a function of both the intensity of imparted swirl (characterized by swirl number) and forcing amplitude. It is observed that for sub-critical VB mode, an increase in the excitation amplitude till a critical value shifts the vortex core centre (particularly, the vortex core moves downstream and radially outwards) leading to drastic fanning-out/widening of the IRZ. This is accompanied by similar to 30% reduction in the recirculation velocity of the IRZ. It is also observed that b < R (R: radial distance from central axis to outer shear layer-OSL). At super-critical amplitudes, the sub-critical IRZ topology transits back (the vortex core retracts upstream and radially inwards) and finally undergoes a transverse shrinkage ((r(vcc))/(r(vcc))(0 Hz) decreases by similar to 20%) when b >= R. In contrast, the vortex core of super-critical breakdown mode consistently spreads radially outwards and is displaced further downstream. Finally, the IRZ fans-out at the threshold excitation amplitude. However, the acoustic response region b is still less than R. This is explained based on the characteristic geometric swirl number (S-G) of the flow regimes. The super-critical flow mode with higher S-G (hence, higher radial pressure drop due to rotational effect which scales as Delta P similar to rho u theta(2) and acts inwards towards the center line) compared to sub-critical state imposes a greater resistance to the radial outward spread of b. As a result, the acoustic energy supplied to the super-critical flow mode increases the degree of acoustic response at the pulsing frequency and energizes its harmonics (evident from power spectra). As a disturbance amplifier, the stronger convective instability mode within the flow structure of super-critical VB causes the topology to widen/fan-out severely at threshold excitation amplitude. (C) 2015 AIP Publishing LLC.

Two bifurcation transitions of the floating half zone convection in a fat liquid bridge of larger Pr

The transient process of the thermocapillary convection was obtained for the large Pu floating half zone by using the method of three-dimensional and unsteady numerical simulation. The convection transits directly from steady and axisymmetric state to oscillatory flow for slender liquid bridge, and transits first from steady and axisymmetric convection to the steady and non-axisymmetric convection, then, secondly to the oscillatory convection for the fatter liquid bridge. This result implies that the volume of liquid bridge is not only a sensitive critical parameter for the onset of oscillation, but also relates to the new mechanism for the onset of instability in the floating half zone convection even in case of large Prandtl number fluid.

Analyses of planetary atmospheres across the spectrum : from Titan to exoplanets

Planetary atmospheres exist in a seemingly endless variety of physical and chemical environments. There are an equally diverse number of methods by which we can study and characterize atmospheric composition. In order to better understand the fundamental chemistry and physical processes underlying all planetary atmospheres, my research of the past four years has focused on two distinct topics. First, I focused on the data analysis and spectral retrieval of observations obtained by the Ultraviolet Imaging Spectrograph (UVIS) instrument onboard the Cassini spacecraft while in orbit around Saturn. These observations consisted of stellar occultation measurements of Titan's upper atmosphere, probing the chemical composition in the region 300 to 1500 km above Titan's surface. I examined the relative abundances of Titan's two most prevalent chemical species, nitrogen and methane. I also focused on the aerosols that are formed through chemistry involving these two major species, and determined the vertical profiles of aerosol particles as a function of time and latitude. Moving beyond our own solar system, my second topic of investigation involved analysis of infra-red light curves from the Spitzer space telescope, obtained as it measured the light from stars hosting planets of their own. I focused on both transit and eclipse modeling during Spitzer data reduction and analysis. In my initial work, I utilized the data to search for transits of planets a few Earth masses in size. In more recent research, I analyzed secondary eclipses of three exoplanets and constrained the range of possible temperatures and compositions of their atmospheres.

Trânsitos ficcionais: um estudo sobre a experiência da viagem na ficção contemporânea

Este trabalho se propõe a analisar a experiência da viagem no contexto da ficção contemporânea brasileira. Para tanto, serão utilizadas as constantes viagens do protagonista do romance Budapeste, de Chico Buarque, para discutir as questões que serão apresentadas. Com a ajuda do pensamento de estudiosos como Bauman, Augé, Schutz, Maffesoli, Deleuze e Guattari, este estudo seguirá os trânsitos ficcionais e as linhas de fuga do protagonista para discutir sobre o modo como o homem contemporâneo vivencia a experiência da mobilidade

Circuito Cineclube: trânsitos audiovisuais

Conforme os percursos que fiz, buscarei mostrar que as práticas cineclubistas se ampliaram em consonância com o alargamento das possibilidades de criação videocinematográficas propiciados pelos avanços da tecnologia da imagem e de sua popularização a partir dos anos 2000, sem se afastar dos seus sentidos iniciais que são a democratização do audiovisual e a organização do público. Sob a designação de cineclube há uma rede de criadores que, em suas ações, realizam, além de obras audiovisuais, espaços-tempos de convivência e intercâmbio de experiências e novas idéias, caracterizando um território identitário, que é o cineclubismo contemporâneo, e que, a despeito dos interesses e elementos de identificação de seus sujeitos, é desfronteirado. Pois assim, mostra-se aberto a contribuições e atravessamentos diversos que de alguma forma envolvem a cultura visual em sua complexa presença na atualidade

Coletivo de trabalho e atividade dos motoboys: gênero profissional, saberes operatórios e riscos da atividade de trabalho

Há cerca de 20 anos, inicia-se no Brasil uma atividade de trabalho nas áreas urbanas: o serviço de motoboys, que vem se tornando comum na distribuição de produtos aos clientes. Em paralelo ao crescimento dessa atividade ocupacional, a quantidade de motociclistas que se acidentam grave ou fatalmente nas vias brasileiras está em pleno crescimento, razão pela qual os motoboys vêm chamando atenção das autoridades de Saúde Pública. Tentando compreender as questões que estão na base e em torno desse fenômeno, inicia-se no país um pequeno, mas consistente, conjunto de produções acadêmicas sobre a profissão. Porém, ainda são poucos os estudos que procuram compreender a atividade de trabalho dos motoboys. Menos ainda, são os que investigam dimensões do coletivo produzidas pelos profissionais (tais como o coletivo de trabalho ou o gênero profissional), bem como seus efeitos na constituição de saberes, discursos, valores e estratégias de enfrentamentos aos diversos contraintes da atividade, em particular as dimensões do risco de acidentes de trabalho. Visando responder especificamente a essa questão, é que se propõe esse trabalho. Para tanto, desenvolveu-se uma pesquisa exploratória em duas perspectivas metodológicas: por um lado um levantamento quantitativo sobre diversos aspectos do trabalho dos motoboys, tais como o perfil do trabalhador, a organização do trabalho e alguns efeitos no trabalhador; essa etapa se deu por meio da aplicação de 189 questionários aplicados em uma amostra proporcional à população identificada de trabalhadores nos principais corredores viários do município de Vitória. Por outro lado, se empreendeu um estudo, baseado nos princípios da Ergologia e em diferentes abordagens clínicas do trabalho, especialmente a Clínica da Atividade e a Psicodinâmica do Trabalho, por meio do qual se pretendeu realizar uma análise da atividade de trabalho em parceria com os trabalhadores, procurando identificar as dimensões do coletivo que são produzidas por meio do trabalho, bem como os saberes e estratégias individuais e coletivas para lidar com as exigências, as pressões, as contradições e as eventualidades do cotidiano. Destaca-se, nessa etapa qualitativa, a realização de uma aproximação etnográfica dos trabalhadores e a utilização das técnicas da autoconfrontação e das instruções ao sósia, essas duas obtidas via Clínica da Atividade. Como resultado, observou-se a existência de inúmeros saberes produzidos e/ou partilhados pelo coletivo, tais como a avaliação dos serviços, a gestão do tempo, o planejamento da rota, a mobilização da rede solidária, a gestão das transgressões, os modos de conduzir, bem como as estratégias coletivas para lidar com o risco, dentre os quais se destacam a exploração positiva do risco e as estratégias baseadas na potência da virilidade, a capacidade de antecipação, ou o cuidado na proteção de si por meio da sinalização da presença do trabalhador em trânsito nas vias. Conclui-se, dessa análise, a existência de um coletivo de trabalho e, mais particularmente, de um gênero profissional em franca constituição. Este, em contrapartida, está eivado de inúmeras contradições e embates que, potencialmente, podem estar atuando para o impedimento da manifestação desse coletivo de trabalho em toda a sua potência