942 research outputs found

    Resonant line transfer in a fog: Using Lyman-alpha to probe tiny structures in atomic gas

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    Motivated by observational and theoretical work which both suggest very small scale (≲1 \lesssim 1\,pc) structure in the circum-galactic medium of galaxies and in other environments, we study Lyman-α\alpha (Lyα\alpha) radiative transfer in an extremely clumpy medium with many "clouds" of neutral gas along the line of sight. While previous studies have typically considered radiative transfer through sightlines intercepting ≲10\lesssim 10 clumps, we explore the limit of a very large number of clumps per sightline (up to fc∼1000f_{\mathrm{c}} \sim 1000). Our main finding is that, for covering factors greater than some critical threshold, a multiphase medium behaves similar to a homogeneous medium in terms of the emergent Lyα\alpha spectrum. The value of this threshold depends on both the clump column density and on the movement of the clumps. We estimate this threshold analytically and compare our findings to radiative transfer simulations with a range of covering factors, clump column densities, radii, and motions. Our results suggest that (i) the success in fitting observed Lyα\alpha spectra using homogeneous "shell models" (and the corresponding failure of multiphase models) hints towards the presence of very small-scale structure in neutral gas, in agreement within a number of other observations; and (ii) the recurrent problems of reproducing realistic line profiles from hydrodynamical simulations may be due to their inability to resolve small-scale structure, which causes simulations to underestimate the effective covering factor of neutral gas clouds.Comment: 18 pages, 21 figures; submitted to A&A; animations available at http://bit.ly/a-in-a-fo

    Barriers to women's access to alongside midwifery units in England

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    Background: Alongside midwifery units (AMUs) are managed by midwives and proximate to obstetric units (OUs), offering a home-like birth environment for women with straightforward pregnancies. They support physiological birth, with fast access to medical care if needed. AMUs have good perinatal outcomes and lower rates of interventions than OUs. In England, uptake remains lower than potential use, despite recent changes in policy to support their use. This article reports on experiences of access from a broader study that investigated AMU organisation and care. Methods: Organisational case studies in four National Health Service (NHS) Trusts in England, selected for variation geographically and in features of their midwifery units. Fieldwork (December 2011 to October 2012) included observations (>100 h); semi-structured interviews with staff, managers and stakeholders (n = 89) and with postnatal women and partners (n = 47), on which this paper reports. Data were analysed thematically using NVivo10 software. Results: Women, partners and families felt welcome and valued in the AMU. They were drawn to the AMUs’ environment, philosophy and approach to technology, including pain management. Access for some was hindered by inconsistent information about the existence, environment and safety of AMUs, and barriers to admission in early labour. Conclusions:Key barriers to AMUs arise through inequitable information and challenges with admission in early labour. Most women still give birth in obstetric units and despite increases in the numbers of women birthing on AMUs since 2010, addressing these barriers will be essential to future scale-up

    Influence of a magnetic field on the viscosity of a dilute gas consisting of linear molecules.

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    The viscomagnetic effect for two linear molecules, N2 and CO2, has been calculated in the dilute-gas limit directly from the most accurate ab initio intermolecular potential energy surfaces presently available. The calculations were performed by means of the classical trajectory method in the temperature range from 70 K to 3000 K for N2 and 100 K to 2000 K for CO2, and agreement with the available experimental data is exceptionally good. Above room temperature, where no experimental data are available, the calculations provide the first quantitative information on the magnitude and the behavior of the viscomagnetic effect for these gases. In the presence of a magnetic field, the viscosities of nitrogen and carbon dioxide decrease by at most 0.3% and 0.7%, respectively. The results demonstrate that the viscomagnetic effect is dominated by the contribution of the jj¯ polarization at all temperatures, which shows that the alignment of the rotational axes of the molecules in the presence of a magnetic field is primarily responsible for the viscomagnetic effect
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