103 resultados para runaway


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Un relevamiento cualitativo y cuantitativo de los avisos de fugas y extravíos de esclavos publicados en La Gaceta Mercantil entre 1823 y 1831 nos permitió analizar pormenorizadamente los atuendos que utilizaba dicho grupo social, sus estados, telas y colores, y cuestionar la visión recibida de los contemporáneos sobre un esclavo mal vestido y harapiento. Comprobamos que vestían mayor variedad y cantidad de prendas, lo cual pudo representar, junto con los ornamentos que complementaron sus ajuares y cierto cuidado en la apariencia personal, una forma de reafirmación de la propia individualidad y el intento de preservación de la identidad de grupo

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Un relevamiento cualitativo y cuantitativo de los avisos de fugas y extravíos de esclavos publicados en La Gaceta Mercantil entre 1823 y 1831 nos permitió analizar pormenorizadamente los atuendos que utilizaba dicho grupo social, sus estados, telas y colores, y cuestionar la visión recibida de los contemporáneos sobre un esclavo mal vestido y harapiento. Comprobamos que vestían mayor variedad y cantidad de prendas, lo cual pudo representar, junto con los ornamentos que complementaron sus ajuares y cierto cuidado en la apariencia personal, una forma de reafirmación de la propia individualidad y el intento de preservación de la identidad de grupo

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Un relevamiento cualitativo y cuantitativo de los avisos de fugas y extravíos de esclavos publicados en La Gaceta Mercantil entre 1823 y 1831 nos permitió analizar pormenorizadamente los atuendos que utilizaba dicho grupo social, sus estados, telas y colores, y cuestionar la visión recibida de los contemporáneos sobre un esclavo mal vestido y harapiento. Comprobamos que vestían mayor variedad y cantidad de prendas, lo cual pudo representar, junto con los ornamentos que complementaron sus ajuares y cierto cuidado en la apariencia personal, una forma de reafirmación de la propia individualidad y el intento de preservación de la identidad de grupo

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The marine nitrogen (N) inventory is thought to be stabilized by negative feedback mechanisms that reduce N inventory excursions relative to the more slowly overturning phosphorus inventory. Using a global biogeochemical ocean circulation model we show that negative feedbacks stabilizing the N inventory cannot persist if a close spatial association of N2 fixation and denitrification occurs. In our idealized model experiments, nitrogen deficient waters, generated by denitrification, stimulate local N2 fixation activity. But, because of stoichiometric constraints, the denitrification of newly fixed nitrogen leads to a net loss of N. This can enhance the N deficit, thereby triggering additional fixation in a vicious cycle, ultimately leading to a runaway N loss. To break this vicious cycle, and allow for stabilizing negative feedbacks to occur, inputs of new N need to be spatially decoupled from denitrification. Our idealized model experiments suggest that factors such as iron limitation or dissolved organic matter cycling can promote such decoupling and allow for negative feedbacks that stabilize the N inventory. Conversely, close spatial co-location of N2 fixation and denitrification could lead to net N loss.

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In contrast to the adjacent parts of the Transantarctic Mountains, the Mesozoic macrofossil record of north Victoria Land remains poorly documented. During the Ninth German Antarctic North Victoria Land Expedition (GANOVEX IX 2005/2006) twelve fossil sites in southern north Victoria Land were discovered and sampled. Fossils from the Triassic to Early Jurassic Section Peak Formation were collected from Archambault Ridge, Anderton Glacier, Skinner Ridge, Timber Peak, Vulcan Hills, Runaway Hills, Section Peak and Shafer Peak. These localities have yielded abundant fossil wood and compressions of horsetails, ferns, and seed ferns. In addition, several beetle elytra were found at Timber Peak. Fossil localities of the overlying Shafer Peak Formation and Exposure Hill-type deposits occur at Shafer Peak and in the Mount Carson area, and have yielded various trace fossils, permineralized wood, leaf compressions, and conchostracans. Two newly discovered fossil sites are associated with the late Early Jurassic Kirkpatrick lava flows. Upright-standing tree trunks have been recorded at Suture Bench, and highly fossiliferous sedimentary interbeds occur at the southwestern end of the Mesa Range. Of special interest is the exquisite fossil preservation at some of the sites. Compression fossils from Timber Peak and Shafer Peak contain well-preserved cuticles, which is very rare in the Antarctic. An Early Jurassic permineralized deposit at Mount Carson contains structurally preserved ferns. Furthermore, the arthropod fossils from sedimentary interbeds at the Mesa Range are preserved in minute detail, including antennae and limb spines of a blattid insect.

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Labor export has been part of Vietnam’s socio-economic development strategy since the beginning of the doi moi era. Recent years, Vietnam has sent about 80,000 workers abroad per year. Vietnam has become a major source country of unskilled foreign workers for high-income East Asian countries. However, in these receiving countries, the desertion rate among Vietnamese workers is quite high, compared with that for workers from other countries. This paper examines the impact of Korean and Japanese policies for receiving foreign workers applied to and implemented in Vietnam, as well as the impact of Vietnamese labor sending system, on the problem of runaway workers.

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Conditions are identified under which analyses of laminar mixing layers can shed light on aspects of turbulent spray combustion. With this in mind, laminar spray-combustion models are formulated for both non-premixed and partially premixed systems. The laminar mixing layer separating a hot-air stream from a monodisperse spray carried by either an inert gas or air is investigated numerically and analytically in an effort to increase understanding of the ignition process leading to stabilization of high-speed spray combustion. The problem is formulated in an Eulerian framework, with the conservation equations written in the boundary-layer approximation and with a one-step Arrhenius model adopted for the chemistry description. The numerical integrations unveil two different types of ignition behaviour depending on the fuel availability in the reaction kernel, which in turn depends on the rates of droplet vaporization and fuel-vapour diffusion. When sufficient fuel is available near the hot boundary, as occurs when the thermochemical properties of heptane are employed for the fuel in the integrations, combustion is established through a precipitous temperature increase at a well-defined thermal-runaway location, a phenomenon that is amenable to a theoretical analysis based on activation-energy asymptotics, presented here, following earlier ideas developed in describing unsteady gaseous ignition in mixing layers. By way of contrast, when the amount of fuel vapour reaching the hot boundary is small, as is observed in the computations employing the thermochemical properties of methanol, the incipient chemical reaction gives rise to a slowly developing lean deflagration that consumes the available fuel as it propagates across the mixing layer towards the spray. The flame structure that develops downstream from the ignition point depends on the fuel considered and also on the spray carrier gas, with fuel sprays carried by air displaying either a lean deflagration bounding a region of distributed reaction or a distinct double-flame structure with a rich premixed flame on the spray side and a diffusion flame on the air side. Results are calculated for the distributions of mixture fraction and scalar dissipation rate across the mixing layer that reveal complexities that serve to identify differences between spray-flamelet and gaseous-flamelet problems.

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The broad host range plasmid RK2 replicates and regulates its copy number in a wide range of Gram-negative bacteria. The plasmid-encoded trans-acting replication protein TrfA and the origin of replication oriV are sufficient for controlled replication of the plasmid in all Gram-negative bacteria tested. The TrfA protein binds specifically to direct repeat sequences (iterons) at the origin of replication. A replication control model, designated handcuffing or coupling, has been proposed whereby the formation of coupled TrfA-oriV complexes between plasmid molecules results in hindrance of origin activity and, consequently, a shut-down of plasmid replication under conditions of higher than normal copy number. Therefore, according to this model, the coupling activity of an initiation protein is essential for copy number control and a copy-up initiation protein mutant should have reduced ability to form coupled complexes. To test this model for plasmid RK2, two previously characterized copy-up TrfA mutations, trfA-254D and trfA-267L, were combined and the resulting copy-up double mutant TFrfA protein TrfA-254D/267L was characterized. Despite initiating runaway (uncontrolled) replication in vivo, the copy-up double-mutant TrfA protein exhibited replication kinetics similar to the wild-type protein in vitro. Purified TrfA-254D, TrfA-267L, and TrfA-254D/267L proteins were then examined for binding to the iterons and for coupling activity using an in vitro ligase-catalyzed multimerization assay. It was found that both single and double TrfA mutant proteins exhibited substantially reduced (single mutants) or barely detectable (double mutant) levels of coupling activity while not being diminished in their capacity to bind to the origin of replication. These observations provide direct evidence in support of the coupling model of replication control.

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Context. During the course of a large spectroscopic survey of X-ray active late-type stars in the solar neighbourhood, we discovered four lithium-rich stars packed within just a few degrees on the sky. Although located in a sky area rich in CO molecular regions and dark clouds, the Cepheus-Cassiopeia complex, these very young stars are projected several degrees away from clouds in front of an area void of interstellar matter. As such, they are very good "isolated" T Tauri star candidates. Aims. We present optical observations of these stars conducted with 1-2 m class telescopes. We acquired high-resolution optical spectra as well as photometric data allowing us to investigate in detail their nature and physical parameters with the aim of testing the "runaway" and "in-situ" formation scenarios. Their kinematical properties are also analyzed to investigate their possible connection to already known stellar kinematic groups. Methods. We use the cross-correlation technique and other tools developed by us to derive accurate radial and rotational velocities and perform an automatic spectral classification. The spectral subtraction technique is used to infer chromospheric activity level in the Hα line core and clean the spectra of photospheric lines before measuring the equivalent width of the lithium absorption line. Results. Both physical (lithium content, chromospheric, and coronal activities) and kinematical indicators show that all stars are very young, with ages probably in the range 10-30 Myr. In particular, the spectral energy distribution of TYC4496-780-1 displays a strong near-and far-infrared excess, typical of T Tauri stars still surrounded by an accretion disc. They also share the same Galactic motion, proving that they form a homogeneous moving group of stars with the same origin. Conclusions. The most plausible explanation of how these "isolated" T Tauri stars formed is the "in-situ" model, although accurate distances are needed to clarify their connection with the Cepheus-Cassiopeia complex. The discovery of this loose association of "isolated" T Tauri stars can help to shed light on atypical formation processes of stars and planets in low-mass clouds.

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Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical models predict the production of high-energy photons by nonthermal radiative processes, but their efficiency is still debated. Aims. We aim to test and explain the possibility of emission from the bow shocks formed by runaway stars traveling through the interstellar medium by using previous theoretical models. Methods. We applied our model to AE Aurigae, the first reported star with an X-ray detected bow shock, to BD+43 3654, in which the observations failed in detecting high-energy emission, and to the transition phase of a supergiant star in the late stages of its life. Results. From our analysis, we confirm that the X-ray emission from the bow shock produced by AE Aurigae can be explained by inverse Compton processes involving the infrared photons of the heated dust. We also predict low high-energy flux emission from the bow shock produced by BD+43 3654, and the possibility of high-energy emission from the bow shock formed by a supergiant star during the transition phase from blue to red supergiant. Conclusions. Bow shocks formed by different types of runaway stars are revealed as a new possible source of high-energy photons in our neighborhood.

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Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical models predict the production of high-energy photons by nonthermal radiative processes, but their efficiency is still debated. Aims. We aim to test and explain the possibility of emission from the bow shocks formed by runaway stars traveling through the interstellar medium by using previous theoretical models. Methods. We applied our model to AE Aurigae, the first reported star with an X-ray detected bow shock, to BD+43 3654, in which the observations failed in detecting high-energy emission, and to the transition phase of a supergiant star in the late stages of its life. Results. From our analysis, we confirm that the X-ray emission from the bow shock produced by AE Aurigae can be explained by inverse Compton processes involving the infrared photons of the heated dust. We also predict low high-energy flux emission from the bow shock produced by BD+43 3654, and the possibility of high-energy emission from the bow shock formed by a supergiant star during the transition phase from blue to red supergiant. Conclusions. Bow shocks formed by different types of runaway stars are revealed as a new possible source of high-energy photons in our neighborhood.

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Este trabalho examina a representação das cidades na obra de Woody Allen. No intuito de compreender a saída do cineasta patrimônio da cidade de Nova York para a Europa, retoma-se criticamente a questão da Era da Lista Negra, das runaway productions e dos blockbusters. Para analisar os filmes de Allen na Europa considera-se importante entender como a cidade de Nova York configura-se no início da carreira do diretor, notadamente, em filmes que estabelecem um contraponto entre o Brooklyn e Manhattan. Em seguida, examina-se a questão crítica fundamental do trabalho: o cartão-postal corporativo na Europa. Nesse sentido, propõe-se a análise dos cartões-postais de Barcelona, Paris e Roma. O filme Vicky Cristina Barcelona adquire centralidade nesta pesquisa por apresentar de maneira exemplar a paisagem postiça da cidade encarcerada sob intervenção corporativa.

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Competitiveness adjustment in struggling southern euro-area members requires persistently lower inflation than in major trading partners, but low inflation worsens public debt sustainability. When average euro-area inflation undershoots the two percent target, the conflict between intra-euro relative price adjustment and debt sustainability is more severe. In our baseline scenario, the projected public debt ratio reduction in Italy and Spain is too slow and does not meet the European fiscal rule. Debt projections are very sensitive to underlying assumptions and even small negative deviations from GDP growth, inflation and budget surplus assumptions can easily result in a runaway debt trajectory. The case for a greater than five percent of GDP primary budget surplus is very weak. Beyond vitally important structural reforms, the top priority is to ensure that euro area inflation does not undershoot the two percent target, which requires national policy actions and more accommodative monetary policy. The latter would weaken the euro exchange rate, thereby facilitating further intra-euro adjustment. More effective policies are needed to foster growth. But if all else fails, the European Central Bank’s Outright Monetary Transactions could reduce borrowing costs.

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Mode of access: Internet.