285 research outputs found

    Extragalactic Results from the Infrared Space Observatory

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    More than a decade ago the IRAS satellite opened the realm of external galaxies for studies in the 10 to 100 micron band and discovered emission from tens of thousands of normal and active galaxies. With the 1995-1998 mission of the Infrared Space Observatory the next major steps in extragalactic infrared astronomy became possible: detailed imaging, spectroscopy and spectro-photometry of many galaxies detected by IRAS, as well as deep surveys in the mid- and far- IR. The spectroscopic data reveal a wealth of detail about the nature of the energy source(s) and about the physical conditions in galaxies. ISO's surveys for the first time explore the infrared emission of distant, high-redshift galaxies. ISO's main theme in extragalactic astronomy is the role of star formation in the activity and evolution of galaxies.Comment: 106 pages, including 17 figures. Ann.Rev.Astron.Astrophys. (in press), a gzip'd pdf file (667kB) is also available at http://www.mpe.mpg.de/www_ir/preprint/annrev2000.pdf.g

    Vocal quality description of senile characters from Hollywood movies

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    PURPOSE: to describe the vocal quality of Hollywood movies characters playing elderly people roles. METHODS: a total of 50 aged character voice samples were used, 11 female and 39 male, from 38 Hollywood movies from the period between 1993 and 2001. Twenty speech therapists performed a perceptual auditory analysis. The listener's task required classifying each character either as elderly or as adult by their speech features, and also assessing their voices following the parameters that are most frequently addressed in the literature as being disordered at an old age. The parameters were hoarseness, vocal fry, breathiness, strain, roughness, vocal weakness, nasal resonance, tremor, vocal modulation, pitch and fundamental frequency stability. RESULTS: after the perceptual auditory analysis we noted that a great number of actors (82%) used senile voices indicating old age, even though not all of them were elderly. The most salient voice set altered was vocal quality (92%), demonstrated by vocal fry (80%), breathiness (54%), strain (38%), hoarseness (30%), and weak voice (28%). The second vocal set most used by the actors for their roles was extensive vocal modulation (44%). It was also observed that vocal instability (64%) was used by the actors. CONCLUSION: it can be concluded from the results that Hollywood movies characterize the elderly characters through evident deviations in vocal quality and modulation, using disordered types of voices and vocal unstable and extensive modulation.OBJETIVO: descrever a qualidade vocal de personagens idosos dos filmes de Hollywood. MÉTODOS: foram colhidas 50 amostras de fala de personagens idosos, 11 do sexo feminino e 39 do masculino, de 38 filmes hollywoodianos dos anos de 1993 a 2001. Através da análise perceptivo-auditiva das amostras de fala, 20 fonoaudiólogos treinados classificaram cada personagem em idoso e não idoso, além de avaliarem as vozes quanto aos seguintes parâmetros citados pela literatura como mais alterados: rouquidão, crepitação, soprosidade, tensão, aspereza, astenia, nasalidade, tremor, modulação, pitch e estabilidade da frequência fundamental. RESULTADOS: após a análise perceptivo-auditiva, foi observado que a grande maioria dos atores (82%) utilizou voz de idoso para representar seus papéis. O marcador mais evidente nas vozes foi alteração na qualidade vocal (92%), demonstrada por crepitação (80%), soprosidade (54%), tensão (38%), rouquidão (30%) e astenia (28%). O segundo marcador mais utilizado pelos atores nas suas representações foi a modulação vocal ampla e variada (44%). Também foram observadas alterações no controle da voz (36%) e instabilidade da frequência fundamental (38%). CONCLUSÃO: a partir dos resultados obtidos pode-se concluir que os filmes de Hollywood caracterizam o idoso através de desvios evidentes na qualidade e modulação da voz, utilizando tipos de vozes alteradas e modulação vocal ampla e instável.Universidade Federal de São Paulo (UNIFESP) Centro de Estudos da VozUNIFESP, Centro de Estudos da VozSciEL

    Functional traits of the world’s late Quaternary large-bodied avian and mammalian herbivores

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    Prehistoric and recent extinctions of large-bodied terrestrial herbivores had significant and lasting impacts on Earth’s ecosystems due to the loss of their distinct trait combinations. The world’s surviving large-bodied avian and mammalian herbivores remain among the most threatened taxa. As such, a greater understanding of the ecological impacts of large herbivore losses is increasingly important. However, comprehensive and ecologically-relevant trait datasets for extinct and extant herbivores are lacking. Here, we present HerbiTraits, a comprehensive functional trait dataset for all late Quaternary terrestrial avian and mammalian herbivores ≥10 kg (545 species). HerbiTraits includes key traits that influence how herbivores interact with ecosystems, namely body mass, diet, fermentation type, habitat use, and limb morphology. Trait data were compiled from 557 sources and comprise the best available knowledge on late Quaternary large-bodied herbivores. HerbiTraits provides a tool for the analysis of herbivore functional diversity both past and present and its effects on Earth’s ecosystems

    Multi-messenger observations of a binary neutron star merger

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    On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

    Coping with Commitment: Projected Thermal Stress on Coral Reefs under Different Future Scenarios

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    BACKGROUND: Periods of anomalously warm ocean temperatures can lead to mass coral bleaching. Past studies have concluded that anthropogenic climate change may rapidly increase the frequency of these thermal stress events, leading to declines in coral cover, shifts in the composition of corals and other reef-dwelling organisms, and stress on the human populations who depend on coral reef ecosystems for food, income and shoreline protection. The ability of greenhouse gas mitigation to alter the near-term forecast for coral reefs is limited by the time lag between greenhouse gas emissions and the physical climate response. METHODOLOGY/PRINCIPAL FINDINGS: This study uses observed sea surface temperatures and the results of global climate model forced with five different future emissions scenarios to evaluate the "committed warming" for coral reefs worldwide. The results show that the physical warming commitment from current accumulation of greenhouse gases in the atmosphere could cause over half of the world's coral reefs to experience harmfully frequent (p> or =0.2 year(-1)) thermal stress by 2080. An additional "societal" warming commitment, caused by the time required to shift from a business-as-usual emissions trajectory to a 550 ppm CO(2) stabilization trajectory, may cause over 80% of the world's coral reefs to experience harmfully frequent events by 2030. Thermal adaptation of 1.5 degrees C would delay the thermal stress forecast by 50-80 years. CONCLUSIONS/SIGNIFICANCE: The results suggest that adaptation -- via biological mechanisms, coral community shifts and/or management interventions -- could provide time to change the trajectory of greenhouse gas emissions and possibly avoid the recurrence of harmfully frequent events at the majority (97%) of the world's coral reefs this century. Without any thermal adaptation, atmospheric CO(2) concentrations may need to be stabilized below current levels to avoid the degradation of coral reef ecosystems from frequent thermal stress events

    Historical Temperature Variability Affects Coral Response to Heat Stress

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    Coral bleaching is the breakdown of symbiosis between coral animal hosts and their dinoflagellate algae symbionts in response to environmental stress. On large spatial scales, heat stress is the most common factor causing bleaching, which is predicted to increase in frequency and severity as the climate warms. There is evidence that the temperature threshold at which bleaching occurs varies with local environmental conditions and background climate conditions. We investigated the influence of past temperature variability on coral susceptibility to bleaching, using the natural gradient in peak temperature variability in the Gilbert Islands, Republic of Kiribati. The spatial pattern in skeletal growth rates and partial mortality scars found in massive Porites sp. across the central and northern islands suggests that corals subject to larger year-to-year fluctuations in maximum ocean temperature were more resistant to a 2004 warm-water event. In addition, a subsequent 2009 warm event had a disproportionately larger impact on those corals from the island with lower historical heat stress, as indicated by lower concentrations of triacylglycerol, a lipid utilized for energy, as well as thinner tissue in those corals. This study indicates that coral reefs in locations with more frequent warm events may be more resilient to future warming, and protection measures may be more effective in these regions

    Multiscale QM/MM modelling of catalytic systems with ChemShell

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    Hybrid quantum mechanical/molecular mechanical (QM/MM) methods are a powerful computational tool for the investigation of all forms of catalysis, as they allow for an accurate description of reactions occurring at catalytic sites in the context of a complicated electrostatic environment. The scriptable computational chemistry environment ChemShell is a leading software package for QM/MM calculations, providing a flexible, high performance framework for modelling both biomolecular and materials catalysis. We present an overview of recent applications of ChemShell to problems in catalysis and review new functionality introduced into the redeveloped Python-based version of ChemShell to support catalytic modelling. These include a fully guided workflow for biomolecular QM/MM modelling, starting from an experimental structure, a periodic QM/MM embedding scheme to support modelling of metallic materials, and a comprehensive set of tutorials for biomolecular and materials modelling
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