4,277 research outputs found

    Unveiling hidden structures in the Coma cluster

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    We have assembled a large data-set of 613 galaxy redshifts in the Coma cluster, the largest presently available for a cluster of galaxies. We have defined a sample of cluster members complete to b26.5=20.0_{26.5}=20.0, using a membership criterion based on the galaxy velocity, when available, or on the galaxy magnitude and colour, otherwise. Such a data set allows us to define nearly complete samples within a region of 1~\Mpc\ radius, with a sufficient number of galaxies per sample to make statistical analyses possible. Using this sample and the {\em ROSAT} PSPC X--ray image of the cluster, we have re-analyzed the structure and kinematics of Coma, by applying the wavelet and adaptive kernel techniques. A striking coincidence of features is found in the distributions of galaxies and hot intracluster gas. The two central dominant galaxies, NGC4874 and NGC4889, are surrounded by two galaxy groups, mostly populated with galaxies brighter than b26.5=17_{26.5}=17 and well separated in velocity space. On the contrary, the fainter galaxies tend to form a single smooth structure with a central peak coinciding in position with a secondary peak detected in X--rays, and located between the two dominant galaxies; we suggest to identify this structure with the main body of the Coma cluster. A continuous velocity gradient is found in the central distribution of these faint galaxies, a probable signature of tidal interactions rather than rotation. There is evidence for a bound population of bright galaxies around other brightest cluster members. Altogether, the Coma cluster structure seems to be better traced by the faint galaxy population, the bright galaxies being located in subclusters. We discuss this evidence in terms of an ongoing accretion of groups onto the cluster.Comment: to appear in A&A, 19 pages, uuencoded gzipped postscript fil

    Physical mechanisms involved in grooved flat heat pipes: experimental and numerical analyses

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    International audienceAn experimental database, obtained with flat plate heat pipes (FPHP) with longitudinal grooves is presented. The capillary pressure measured by confocal microscopy and the temperature field in the wall are presented in various experimental conditions (vapour space thickness, filing ratio, heat transfer rate, tilt angle, fluid). Coupled hydrodynamic and thermal models are developed. Experimental results are compared to results of numerical models. Physical mechanisms involved in grooved heat pipes are discussed, including the boiling limit and the effect of the interfacial shear stress. Finally, recommendations for future experimental and theoretical research to increase the knowledge on FPHP are discussed

    Combined effects of the filling ratio and the vapour space thickness on the performance of a flat plate heat pipe

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    International audienceAn experimental study of a flat plate heat pipe (FPHP) is presented. Temperature fields in the FPHP are measured for different filling ratios, heat fluxes and vapour space thicknesses. The system is hermetically sealed with a transparent plate for meniscus curvature radius observations by confocal microscopy. Experimental results show that the liquid distribution in the FPHP - and thus its thermal performance - depends strongly on both the filling ratio and the vapour space thickness. A small vapour space thickness induces liquid retention and thus reduces the thermal resistance of the system. Nevertheless, the vapour space thickness influences the level of the meniscus curvature radii in the grooves and hence reduces the maximum capillary pressure. As a result, it has to be carefully optimised to improve the performance of the FPHP. In all the cases, the optimum filling is in the range one to two times the total volume of the grooves. A theoretical approach, in non working conditions, has been developed to model the distribution of the liquid inside the FPHP in function of the filling ratio and the vapour space thickness

    Selection genetique sur la reponse au stress et stress a l'abattage: consequences sur le proteome musculaire et lien avec la qualite de la chair chez la truite arc-en-ciel.

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    L'origine génétique des animaux est un des facteurs déterminants des caractéristiques des poissons en élevage (croissance, morphologie…) et de la qualité de leur chair. Une sélection divergente, basée sur la réponse individuelle de truite, en terme de niveau plasmatique de cortisol, suite à un stress aigu de confinement, a permis de montrer que ce paramètre est héritable, et d'obtenir des familles de truites présentant des niveaux de réponse à un stress aigu bien distincts (Pottinger et Carrick, 1999). Les animaux de ces familles divergentes ont été caractérisés pour leur croissance, qui s'avère meilleure pour les poissons répondant faiblement au stress, leur morphologie, et la qualité de leur chair. Les poissons répondant faiblement au stress présentent une chair moins lumineuse, plus jaune, et une résistance mécanique moindre associée à des fibres musculaires plus grosses et une teneur en lipides plus importante (Lefèvre et al., 2008a). Un stress au moment de l'abattage modifie le métabolisme post-mortem et conduit, la plupart du temps chez les salmonidés, à une chair moins ferme et plus pale (Lefèvre et al., 2008b). Un tel effet a été confirmé dans cette expérimentation de façon similaire pour les deux souches sélectionnées. Les protéines permettant d’expliquer potentiellement ces différences de qualité ne sont pas connues. L'objectif de ce travail était d'identifier les protéines différentiellement exprimées entre les deux souches sélectionnées et ayant subies ou non un stress de confinement juste avant l'abattage et de faire le lien avec les paramètres de qualité déjà mesurés

    Quels paysages pour demain ? Résumé

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    Enhancement of ferromagnetism by nickel doping in the 112 cobaltite EuBaCo2O5.50

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    The study of the ordered oxygen deficient perovskite EuBaCo2-xNixO5.50 shows that the doping of cobalt sites by nickel induces a strong ferromagnetic component at low temperature in the antiferromagnetic matrix of EuBaCo2O5.50. This system exhibits indeed phase separation, i.e. consists of ferromagnetic domains embedded in the antiferromagnetic matrix of EuBaCo2O5.50. Besides, a magnetic transition is observed for the first time at 40K in the undoped and nickel doped phases, which can be attributed to the ferromagnetic ordering of the Eu3+ moments below this temperature. Moreover sharp ultra magnetization multisteps are observed below 5K, characteristic of motion of domain walls in a strong pinning system and very different from any metamagnetic transition
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