What Makes the Family of Barred Disc Galaxies So Rich: Damping Stellar Bars in Spinning Haloes

We model and analyse the secular evolution of stellar bars in spinning dark matter (DM) haloes with the cosmological spin lambda ~ 0 -- 0.09. Using high-resolution stellar and DM numerical simulations, we focus on angular momentum exchange between stellar discs and DM haloes of various axisymmetric shapes --- spherical, oblate and prolate. We find that stellar bars experience a diverse evolution which is guided by the ability of parent haloes to absorb angular momentum lost by the disc through the action of gravitational torques, resonant and non-resonant. We confirm the previous claim that dynamical bar instability is accelerated via resonant angular momentum transfer to the halo. Our main findings relate to the long-term, secular evolution of disc-halo systems: with an increasing lambda, bars experience less growth and dissolve after they pass through the vertical buckling instability. Specifically, with an increasing halo spin, (1) The vertical buckling instability in stellar bars colludes with inability of the inner halo to absorb angular momentum --- this emerges as the main factor weakening or destroying bars in spinning haloes; (2) Bars lose progressively less angular momentum, and their pattern speeds level off; (3) Bars are smaller, and for lambda >= 0.06 cease their growth completely following buckling; (4) Bars in lambda > 0.03 haloes have ratio of corotation-to-bar radii, R_CR / R_b > 2, and represent so-called slow bars which do not show offset dust lanes. We provide a quantitative analysis of angular momentum transfer in disc-halo systems, and explain the reasons for absence of growth in fast spinning haloes and its observational corollaries. We conclude that stellar bar evolution is substantially more complex than anticipated, and bars are not as resilient as has been considered so far.Comment: 15 pages., 11 figures, MNRAS, in pres

Evolution of Barred Galaxies in Spinning Dark Matter Halos: High Resolution N-body Simulations at DLX

Observations show that galaxies are dominated by stellar disks immersed in much more massive, slowly tumbling dark matter (DM) halos. Large fraction of galactic disks, at least 75%, are barred (see Hubble Fork on the right). Stellar bars form either via spontaneous break of axial symmetry or via galaxy interactions. The formation and evolution of stellar bars is not fully understood. Stellar bar evolution is highly nonlinear and cannot be treated analytically. The main approach to study these disk-halo systems is via numerical simulations, whose goal is to explain why galaxies have such a wide range of morphologies as shown on the Hubble Fork diagram

On the Potential for Saturated Buffers in Northwest Ohio to Remediate Nutrients from Agricultural Runoff

Nutrient loading from nonpoint source runoff in the Midwest has emerged as one of the largest threats to water quality as the frequency of harmful algal blooms, hypoxic zones, and issues associated with human-resource interactions have risen abruptly over the past several decades. In this study, a saturated buffer ~500 m in length located in the western basin of the Lake Erie watershed was evaluated for its potential to reduce edge of field runoff and nutrient loading. Saturated buffers reduce runoff by routing subsurface tile drainage water into the riparian zone, providing an opportunity for drainage volume as well as nutrient reduction of runoff waters. Over a 12-month study period, controlled drainage was used to redirect nearly 25% of the total tile flow into the riparian zone from a subwatershed in corn/soybean rotation with near complete reductions of dissolved nitrogen and phosphorus from tile inflows averaging 4.7 and 0.08 mg/L, respectively, as well as total reduction of suspended sediments (average 10.4 mg/L). This study provides additional evidence that riparian areas are an important part of nutrient reduction strategies as they can act as both controlled drainage points by raising water tables in fields as well as nutrient sinks which couple to help mitigate nutrient runoff in the region

Unidentified infrared bands and the formation of PAHs around carbon stars

Although unidentified infrared bands (UIBs) have been observed in many astrophysical environments, there is one notable exception: carbon (C) stars. Only a handful of C stars have been shown to emit UIBs and most have hot companions. This makes C stars with hot companions an ideal location to investigate the emitters of the UIBs. PAHs are excited by absorption of single photons whose energy is then distributed over the whole molecule. These molecules then emit the energy at the characteristic wavelengths, but the precise wavelengths and strength ratios depend on the size, composition and charge state of the individual PAHs. Furthermore, the wavelength of photons needed to excite PAHs depends on their size and charge state. While small PAHs undoubtedly need higher energy (UV) photons, it has been suggested that large or ionized PAHS (\u3e100 C atoms) can be excited by visible or even near-IR photons. The lack of PAH emission from single carbon stars suggests that either PAHs do not form around C stars or that only small neutral grains form, which cannot be excited by a C star\u27s radiation field. There are two competing formation mechanisms for PAHs around C stars: (1) bottom-up where acetylene molecules react to form aromatic rings, building up to PAHs; or (2) top-down, where small carbon grains react with H atoms and desorb PAHs Using spatially resolved spectroscopic observations from Gemini/Michelle, of five carbon stars with hot companions, we investigate the circumstance under which PAH emission occurs and try to discriminate between formation mechanisms. © 2008 International Astronomical Union

Comparison of cause of death between ANZDATA and the Australian national death index.

Aim: The aim of the present study was to understand the differences in how cause of death for patients receiving renal replacement therapy in Australia is recorded in The Australian and New Zealand Dialysis and Transplant Registry (ANZDATA) compared to the National Death Index (NDI). Methods: Data linkage was performed between ANZDATA and NDI for all deaths in the period 1980-2013. Cause of death was classified according to ICD-10 chapter. Overall and chapter specific agreement were assessed using the Kappa statistic. Descriptive analysis was used to explore differences where there was disagreement on primary cause of death. Results: The analysis cohort included 28 675 patients. Ninety five percent of ANZDATA reported deaths fell within +/- 3 days of the date recorded by NDI. Circulatory death was the most common cause of death in both databases (ANZDATA 48%, NDI 32%). Overall agreement at ICD chapter level of primary cause was poor (36%, kappa 0.22). Agreement was best for malignancy (kappa 0.71). When there was disagreement on primary cause of death these were most commonly coded as genitourinary (35%) and endocrine (25.0%) in NDI, and circulatory (39%) and withdrawal (24%) in ANZDATA. Sixty-nine percent of patients had a renal related cause documented as either primary or a contributing cause of death in the NDI. Conclusion: There is poor agreement in primary cause of death between ANZDATA and NDI which is in part explained by the absence of diabetes and renal failure as causes of death in ANZDATA and the absence of 'withdrawal' in NDI. These differences should be appreciated when interpreting epidemiological data on cause of death in the Australian end stage kidney disease population

Rapid Seismic Waveform Modeling and Inversion with Universal Neural Operators

Seismic waveform modeling is a powerful tool for determining earth structure models and unraveling earthquake rupture processes, but it is computationally expensive. We introduce a scheme to vastly accelerate these calculations with a recently developed machine learning paradigm called the neural operator. Once trained, these models can simulate a full wavefield for arbitrary velocity models at negligible cost. We use a U-shaped neural operator to learn a general solution operator to the 2D elastic wave equation from an ensemble of numerical simulations performed with random velocity models and source locations. We show that full waveform modeling with neural operators is nearly two orders of magnitude faster than conventional numerical methods, and more importantly, the trained model enables accurate simulation for arbitrary velocity models, source locations, and mesh discretization, even when distinctly different from the training dataset. The method also enables efficient full-waveform inversion with automatic differentiation

Immunoregulatory Potential of Exosomes Derived from Cancer Stem Cells.

Head and neck squamous cell carcinomas (HNSCCs) are malignancies that originate in the mucosal lining of the upper aerodigestive tract. Despite advances in therapeutic interventions, survival rates among HNSCC patients have remained static for years. Cancer stem cells (CSCs) are tumor-initiating cells that are highly resistant to treatment, and are hypothesized to contribute to a significant fraction of tumor recurrences. Consequently, further investigations of how CSCs mediate recurrence may provide insights into novel druggable targets. A key element of recurrence involves the tumor's ability to evade immunosurveillance. Recent published reports suggest that CSCs possess immunosuppressive properties, however, the underlying mechanism have yet to be fully elucidated. To date, most groups have focused on the role of CSC-derived secretory proteins, such as cytokines and growth factors. Here, we review the established immunoregulatory role of exosomes derived from mixed tumor cell populations, and propose further study of CSC-derived exosomes may be warranted. Such studies may yield novel insights into new druggable targets, or lay the foundation for future exosome-based diagnostics

4th International Conference - Sexuality and Cancer Breast Cancer

Breast cancer patients and the artists involved in the highly innovative ComMA research programme led an experiential workshop attended by 100 health professional delegates. The experiential workshop explained how patients and artists together explored sexual problems encountered following breast cancer treatment. This novel and highly collaborative approach empowered patients to use art and new forms of artistic expression as an alternative language to express and communicate their feelings of emotional and physical trauma using visual metaphors. ComMA enabled patients to explore and express their feelings through the use of collage, drawing on items such as gowns, which had a deep meaning in the context of their treatment, to enable them to express their feelings openly. Work co-produced by the artists and patients was shared at the workshop to challenge health professionals to understand the patients’ concerns, insecurities and difficulties in communicating their sexual and relationship problems

‘Subjects and Objects: Material Expressions of Love and Loyalty in Seventeenth-Century England’, in special section on ‘Loyalties and Allegiances in Early Modern England’ in Journal of British Studies Vol. 48: 4 (October, 2009)

This article investigates how and where the emotive relations between subject and state were forged and how these ideas were manifested in early modern England. McShane describes an affective economy of loyalty, embodied in cheap and accessible political commodities: decorated objects made of clay, metals, and paper, on which precious household resources of time, money and emotion were spent. She argues that by engendering, inculcating and insinuating codes of political love into people’s ‘emotional, sensual, representational, and communicative’ lives, ‘loyal’ goods acted as vehicles and texts for what Victoria Kahn describes as ‘the supplementary role of the passions’ in ‘forging political obligation’ and the reformulation of ‘the duty to love’ of both subject and king in 17th-century England. McShane’s research contributes to a growing theme in scholarship, namely the active consumption of politically significant goods. This essay extends the range of objects under examination to include quotidian household items, shedding light on the dissemination and construction of early modern loyalty across a much wider social scale. The research draws on an extensive survey of collections held at the V&A, the Museum of London, Ashmolean Museum, Fitzwilliam Museum and Burrell Collection. Importantly, by putting illustrated print products back together with other political commodities in the early modern home, creating a broad archive of objects and text-objects where each informs the other, McShane’s approach challenges the typical social historical methodology, which uses material culture as merely illustrative of textual sources. This article was part of a special section on loyalty and allegiance in early modern England, co-edited by McShane with Dr Ted Vallance for one of the leading scholarly journals in the field. The material was drawn from a workshop on the topic held at the University of Liverpool funded by the British Academy, University of Liverpool and the Scouloudi Foundation (2007)