6,598 research outputs found
The ortho-para H2 distribution on Uranus: Constraints from the collision-induced 3-0 dipole band and 4-0 S(0) and S(1) quadrupole line profiles
Recent high quality spectral observations have allowed the derivation of constraints on the atmospheric structure of Uranus. The present analysis, which is based on the detailed modeling of a broadband geometric albedo spectrum and high resolution observations of the H2 4-0 quadrupole and 6818.9-A CH4 features, yields (1) a family of models which parameterize an upper tropospheric haze layer, (2) a lower, optically infinite cloud at a given pressure level, (3) the cloud-level methane molar fraction, and (4) the mean ortho/para ratio in the visible atmosphere. The single scattering albedo of atmospheric aerosols exhibits a steep darkening between 5890 and 6040 A
Magnetic order and spin dynamics across a ferromagnetic quantum critical point: SR investigations of YbNi(PAs)
In the quasi-1D heavy-fermion system YbNi(PAs) the
presence of a ferromagnetic (FM) quantum critical point (QCP) at with unconventional quantum critical exponents in the thermodynamic
properties has been recently reported. Here, we present muon-spin relaxation
(SR) experiments on polycrystals of this series to study the magnetic
order and the low energy 4-electronic spin dynamics across the FM QCP. The
zero field SR measurements on pure YbNi(P proved static long
range magnetic order and suggested a strongly reduced ordered Yb moment of
about 0.04. With increasing As substitution the ordered moment is
reduced by half at and to less than 0.005 at . The
dynamic behavior in the SR response show that magnetism remains
homogeneous upon As substitution, without evidence for disorder effect. In the
paramagnetic state across the FM QCP the dynamic muon-spin relaxation rate
follows 1/ with . The critical fluctuations are very slow and are even becoming slower
when approaching the QCP.Comment: 6 pages, 4 figure
Children’s social experiences with peers and friends during primary school mealtimes
Mealtimes have rarely been considered outside a healthy eating agenda yet may be important social contexts for children’s social, emotional and moral development. Little research has examined the social value of time spent in the school lunch room. This study examined the nature of children’s interactions, activities and experiences of mealtimes and their perceptions of the value of social experiences during these times. A total of 316 9-10-year-old pupils (53% girls) from 11 classes in 4 schools completed closed response questionnaires and 16 children were subsequently interviewed to provide detailed information about the nature of their mealtime experiences, interactions and activities with peers and how these relate to feelings about school. Findings indicate that most children enjoy mealtimes because of the opportunity they provide to be with and converse with friends and other peers about the issues that are significant to them. These social occasions overlap with playground life but are distinctive and afford children different social opportunities and activities. The relative freedom offered in these settings make them important sites for peer relations processes and co-construction of peer culture. Findings are discussed in the light of suggestions that mealtimes should be managed for social and educational purposes
Development and validation of a chemostat gut model to study both planktonic and biofilm modes of growth of Clostridium difficile and human microbiota
Copyright: 2014 Crowther et al. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.The human gastrointestinal tract harbours a complex microbial community which exist in planktonic and sessile form. The degree to which composition and function of faecal and mucosal microbiota differ remains unclear. We describe the development and characterisation of an in vitro human gut model, which can be used to facilitate the formation and longitudinal analysis of mature mixed species biofilms. This enables the investigation of the role of biofilms in Clostridium difficile infection (CDI). A well established and validated human gut model of simulated CDI was adapted to incorporate glass rods that create a solid-gaseous-liquid interface for biofilm formation. The continuous chemostat model was inoculated with a pooled human faecal emulsion and controlled to mimic colonic conditions in vivo. Planktonic and sessile bacterial populations were enumerated for up to 46 days. Biofilm consistently formed macroscopic structures on all glass rods over extended periods of time, providing a framework to sample and analyse biofilm structures independently. Whilst variation in biofilm biomass is evident between rods, populations of sessile bacterial groups (log10 cfu/g of biofilm) remain relatively consistent between rods at each sampling point. All bacterial groups enumerated within the planktonic communities were also present within biofilm structures. The planktonic mode of growth of C. difficile and gut microbiota closely reflected observations within the original gut model. However, distinct differences were observed in the behaviour of sessile and planktonic C. difficile populations, with C. difficile spores preferentially persisting within biofilm structures. The redesigned biofilm chemostat model has been validated for reproducible and consistent formation of mixed species intestinal biofilms. This model can be utilised for the analysis of sessile mixed species communities longitudinally, potentially providing information of the role of biofilms in CDI.Peer reviewe
Ruling Out Possible Secondary Stars to Exoplanet Host Stars Using the CHARA Array
Of the over 450 exoplanets known to date, more than 420 of them have been
discovered using radial velocity studies, a method that tells nothing about the
inclination of the planet's orbit. Because it is more likely that the companion
is a planetary-mass object in a moderate- to high-inclination orbit than a
low-mass stellar object in a nearly face-on orbit, the secondary bodies are
presumed to be planets. Interferometric observations allow us to inspect the
angular diameter fit residuals to calibrated visibilities in order to rule out
the possibility of a low-mass stellar companion in a very low-inclination
orbit. We used the Center for High Angular Resolution Astronomy (CHARA) Array
interferometer to observe 20 exoplanet host stars and considered five potential
secondary spectral types: G5 V, K0 V, K5 V, M0 V, and M5 V. If a secondary star
is present and is sufficiently bright, the effects of the added light will
appear in interferometric observations where the planet will not. All secondary
types could be eliminated from consideration for 7 host stars and no secondary
stars of any spectral type could be ruled out for 7 more. The remaining 6 host
stars showed a range of possible secondary types.Comment: Accepted for publication in the Astronomical Journa
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