10,105 research outputs found

    On the Influence of X-Ray Galaxy Clusters in the Fluctuations of the Cosmic Microwave Background

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    The negative evolution found in X--ray clusters of galaxies limits the amount of available hot gas for the inverse Compton scattering of the Cosmic Microwave Background (the Sunyaev--Zel'dovich effect). Using a parametrisation of the X-ray luminosity function and its evolution in terms of a coalescence model (as presented in the analysis of a flux limited X-ray cluster sample by Edge et al. 1990), as well as a simple virialised structure for the clusters (which requires a gas to total mass fraction \approxgt 0.1 in order to reproduce observed properties of nearby clusters) we show that the Compton distortion yy parameter is about two orders of magnitude below the current FIRAS upper limits. Concerning the anisotropies imprinted on arcmin scales they are dominated by the hottest undetected objects. We show that they are negligible ({\Delta T\over T}\approxlt 10^{-7}) at wavelengths \lambda\approxgt 1~mm. At shorter wavelengths they become more important (ΔTT∼10−6{\Delta T\over T}\sim 10^{-6} at λ∼0.3\lambda\sim 0.3~mm), but in fact most clusters will produce an isolated and detectable feature in sky maps. After removal of these signals, the fluctuations imprinted by the remaining clusters on the residual radiation are still much smaller. The conclusion is that X-ray clusters can be ignored as sources of Cosmic Microwave Background fluctuations.Comment: 20 pages Plain Tex, 7 figures available upon request,UCAST-94-0

    Soft versus Hard X-ray emission in AGN: partial covering and warm plus cold absorber models

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    We analyse the ROSAT PSPC hardness ratio and the 0.5-2 keV to 2-10 keV flux ratio of 65 Active Galactic Nuclei (AGN) for which there are both ROSAT archival observations available and 2-10 keV fluxes, mostly from the HEAO-1 MC-LASS survey. We conclude that the simplest spectral model for the AGN that can accommodate the variety of X-ray colours obtained is a standard power law (with energy spectral index α∼0.9\alpha\sim 0.9) plus a ∼0.1\sim 0.1 keV black body both partially absorbed. In our sample, type 1 AGN require an absorbing column around 1022 cm−210^{22}\, {\rm cm}^{-2} with covering fractions between 20 and 100\%, while type 2 AGN display larger columns and ∼100%\sim 100\% coverage. This simple model also provides a good link between soft and hard AGN X-ray luminosity functions and source counts. We also consider a warm absorber as an alternative model to partial covering and find that the the presence of gas in two phases (ionized and neutral) is required.Comment: 10 pages, Latex (mn.sty), 1 table, 5 figures included (epsf), postscript version also available via anonymous ftp at ftp://astsun1.unican.es/pub/ceballos/ . Accepted for publication in MNRA

    X-ray sources as tracers of the large-scale structure in the Universe

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    We review the current status of studies of large-scale structure in the X-ray Universe. After motivating the use X-rays for cosmological purposes, we discuss the various approaches used on different angular scales including X-ray background multipoles, cross-correlations of the X-ray background with galaxy catalogues, clustering of X-ray selected sources and small-scale fluctuations and anisotropies in the X-ray background. We discuss the implications of the above studies for the bias parameter of X-ray sources, which is likely to be moderate for X-ray selected AGN and the X-ray background (~1-2). We finally outline how all-sky X-ray maps at hard X-rays and medium surveys with large sky coverage could provide important tests for the cosmological models.Comment: Invited review presented at the Workshop X-ray Astronomy'99: Stellar endpoints, AGN and the diffuse X-ray background (Astrophys Lett and Comm

    Methods And Systems For Enhancing Feed-conversion-ratio In Animals Using Mobile Enzyme Sequestration Platforms (MSEP)

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    A method for enhancing the enzymatic efficiency of an enzyme added to poultry feed for a living subject, comprises adding a cellulose-degrading enzyme to a mobile enzyme sequestration platform (MESP) so as to form an enzyme-MESP complex; adding the enzyme-MESP complex to poultry feed for a living subject; the enzyme efficiency of the cellulose-degrading enzyme of the enzyme-MESP complex after being exposed to a first adverse environment for a first period of time is at least 50% higher than the enzyme efficacy of the cellulose-degrading enzyme independent of the MESP being exposed to the first adverse environment for the first period of time

    Methods And Systems For Enhancing Feed-conversion-ratio In Animals Using Mobile Enzyme Sequestration Platforms (MSEP)

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    A method for enhancing the enzymatic efficiency of an enzyme added to poultry feed for a living subject, comprises adding a cellulose-degrading enzyme to a mobile enzyme sequestration platform (MESP) so as to form an enzyme-MESP complex; adding the enzyme-MESP complex to poultry feed for a living subject; the enzyme efficiency of the cellulose-degrading enzyme of the enzyme-MESP complex after being exposed to a first adverse environment for a first period of time is at least 50% higher than the enzyme efficacy of the cellulose-degrading enzyme independent of the MESP being exposed to the first adverse environment for the first period of time

    Adjustment of Status for Alien Material Witnesses: Is It Coming Three Years Too Late?

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    Los estímulos del comportamiento de los londinenses en sus compras impulsivas de productos de moda

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    This paper explores the stimuli behind fashion-oriented impulse purchases within physicalshopping environments. The main focus of the study is the stimuli behind ‘emotional’ and‘rational’ consumer’s responses. The primary qualitative data was collected by indepthinterview methodology in a sample of 10 workingwomen from London aged between 25and 35 years. Findings mainly suggest that fashion-oriented impulse purchases, especiallyfor clothing,are influenced by a wide variety of stimuli/responses in a similar way asplanned purchases. However, there are specific stimuli/responses that trigger impulsebuying in a higher degree for the studied sample.Este documento explora los estímulos involucrados en las compras impulsivas de productos de moda dentro de ambientes físicos de compra. El principal foco de este estudio son los estímulos que generan respuestas ‘emocionales’ y ‘racionales’ en el consumidor.Los datos cualitativos primarios fueron recolectados utilizando la metodología de entrevistas a profundidad en una muestra de 10 mujeres trabajadoras en Londres con edades entre 25 y 35 años. Los resultados principalmente sugieren que las compras impulsivas de productos relacionados con moda, especialmente vestuario, pueden ser influenciadas por una gran variedad de estímulos/respuesta de manera similar a las compras planeadas. Sin embargo, se encontraron específicos estímulos/respuesta que estimulanlas compras impulsivas en un mayor nivel para la muestra estudiada
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