9,957,895 research outputs found

    Expérience vécue par les parents lors de l'hospitalisation d'un très grand prématuré de moins de 28 semaines: revue de littérature étoffée

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    Un très grand prématuré de moins de 28 semaines hospitalisé en néonatologie présente de nombreuses complications liées à son immaturité. De plus, les risques de séquelles sévères qu’il pourra présenter dans sa vie future, ainsi que le risque de décès ne sont pas à négliger. Les parents sont donc confrontés à des moments très angoissants durant cette hospitalisation. Pour offrir à ces parents un accompagnement adéquat, l’infirmière devra explorer leur expérience face à cette situation

    IMPURITY TRAPPING EFFECTS IN THE LOCALIZATION OF MUONS IN SOLIDS

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    Muon spin rotation ( mu SR) experiments are now regularly used to study solids and solid-state processes. The interpretation of mu SR data is usually based on a 'standard' picture in which the muons localise randomly in the solid, and then diffuse, possibly encountering impurities. There remain some important cases where no satisfactory interpretation results. For some of these anomalous systems the authors propose an alternative picture in which the two different factors are the importance of metastable (free muon) excited states, and the role of impurities in causing localisation. They show this allows a possible explanation of results for Al:Mn and demonstrate that elastic strain fields of defects may be a major factor in influencing localisation. They also propose a new mechanism for delayed self-trapping

    Quand les adolescents imaginent le site web de leur bibliothèque publique

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    Quelques bibliothèques possèdent un site web dont certaines pages sont réservées aux adolescents. D’autres leur proposent un large panel d’activités, mais restent discrètes quant à leur visibilité en ligne. La littérature reste assez modeste autour du thème des adolescents et des sites web de bibliothèque. De leur côté, les adolescents interrogés s’en font une représentation très limitée et le réduisent à la mise en ligne du catalogue. Construire, avec eux, des pages dédiées aux adolescents pour le site web d’une bibliothèque publique permet de connaître leurs attentes et leurs besoins. En faisant participer activement ce public à la création et à l’entretien de son site, la bibliothèque pourra lui faire connaître ses services, son fonds et son savoir-faire. C’est à deux reprises que les adolescents ont été entendus : lors de focus groups, afin de créer le contenu et lors de tests utilisateurs, pour vérifier que leurs idées ont été comprises. Comme l’imagination et la discussion suffisent parfois à faire naître des idées intéressantes, des prototypes de pages ont pu ainsi être construits et améliorés

    Photometry and dynamics of the minor mergers AM\,1228-260 and AM\,2058-381

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    We investigate interaction effects on the dynamics and morphology of the galaxy pairs AM\,2058-381 and AM\,1228-260. This work is based on rr' images and long-slit spectra obtained with the Gemini Multi-Object Spectrograph at the Gemini South Telescope. The luminosity ratio between the main (AM\,2058A) and secondary (AM\,2058B) components of the first pair is a factor of \sim 5, while for the other pair, the main (AM\,1228A) component is 20 times more luminous than the secondary (AM\,1228B). The four galaxies have pseudo-bulges, with a S\'ersic index n<2n<2. Their observed radial velocities profiles (RVPs) present several irregularities. The receding side of the RVP of AM\,2058A is displaced with respect to the velocity field model, while there is a strong evidence that AM\,2058B is a tumbling body, rotating along its major axis. The RVPs for AM\,1228A indicate a misalignment between the kinematic and photometric major axes. The RVP for AM\,1228B is quite perturbed, very likely due to the interaction with AM\,1228A. NFW halo parameters for AM\,2058A are similar to those of the Milky Way and M\,31. The halo mass of AM\,1228A is roughly 10\% that of AM\,2058A. The mass-to-light (M/L) of AM\,2058 agrees with the mean value derived for late-type spirals, while the low M/L for AM\,1228A may be due to the intense star formation ongoing in this galaxy.Comment: 20 pages, 10 figures, accepted for publication in MNRA

    On the Implementation of AM/AM AM/PM Behavioral Models in System Level Simulation

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    The use of nonlinear device behavioral models offers an economical way of simulating the performance of complex communication systems. A concrete method for implementing the AM/AM AM/PM behavioral model in system level simulation using ADS is developed. This method seamlessly tansfers the data from the circuit level simulation to system level simulation, where the AM/AM AM/PM model is automatically built. The methodology is extendible for use in other software packages or between different software packages

    Suitability of Mycorrhiza-Defective Rice and Its Progenitor for Studies on the Control of Nitrogen Loss in Paddy Fields via Arbuscular Mycorrhiza

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    Employing mycorrhiza-defective mutants and their progenitors does not require inoculation or elimination of the resident microbial community in the experimental study of mycorrhizal soil ecology. We aimed to examine the suitability of mycorrhiza-defective rice (non-mycorrhizal, Oryza sativa L., cv. Nipponbare) and its progenitor (mycorrhizal) to evaluate nitrogen (N) loss control from paddy fields via arbuscular mycorrhizal (AM) fungi. We grew the two rice lines in soils with the full community of AM fungi and investigated root AM colonization. In the absence of AM fungi, we estimated rice N content, soil N concentration and microbial community on the basis of phospholipid fatty acids; we also quantified N loss via NH3 volatilization, N2O emission, runoff and leaching. In the presence of AM fungi, we did not find any evidence of AM colonization for non-mycorrhizal rice while mycorrhizal rice was colonized and percentage of root colonization was 17–24%. In the absence of AM fungi, the two rice lines had similar N content, soil N concentration and microbial community. Importantly, there was no significant difference in N loss via all the four pathways between mycorrhizal and non-mycorrhizal systems. This mycorrhizal/non-mycorrhizal rice pair is suitable for further research on the role of AM fungi in the control of soil N loss in paddy fields
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