42 research outputs found

    SAGA Vol. 82 / 2018-2019

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    https://digitalcommons.augustana.edu/saga/1004/thumbnail.jp

    A Viennese in London: English Reception

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    In a culture conducive to refining his compositions, Haydn was able to find success through his patrons and musical techniques. London was the largest musical city at the time, where advertising played a key role in the attendance at concerts. Haydn attended performances there which educated him on London’s music. His patrons (such as violinist Johann Peter Salomon and author Charles Burney) were immensely helpful in his growing musical career in London. Haydn’s shift in compositional style accordingly reflected his stay in London. He combined the music he heard in the city with his own musical language to create his new style. Through studying London’s concert life and Haydn’s interaction with it, one can understand why Haydn’s style changed while within a new city

    Between Two Worlds

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    “Original Sin”—evocative and powerful words, but what if they were applied to one of the world’s most popular fairy tales? This thesis explores Snow White in the context of the Seven Deadly Sins and the grand fall of Adam and Eve. The forbidden fruit manifests itself in different ways, pulling the prim and proper princess into places she never could have imagined. But what of the Wicked Queen, here known as Lilith? She too feels the bite of the world’s sick sense of humor, exacting revenge on those who have wronged her. Are these poems about them? Or are they about the author? Perhaps they are both: the innocent children learn quickly of life’s cruelty, handling it with equal parts grace and selfishness. Dive into the minds of Lilith and Snow White as they explore what it means to be themselves in a world that doesn’t care if they end up happy

    The low redshift Lyman-α\alpha Forest as a constraint for models of AGN feedback

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    We study the low redshift Lyman-α\alpha Forest in the Illustris and IllustrisTNG (TNG) cosmological simulations to demonstrate their utility in constraining aspects of sub-grid models of feedback from active galactic nuclei (AGN). The two simulations share an identical Ultraviolet Background prescription and similar cosmological parameters, but TNG features an entirely reworked AGN feedback model. Therefore a comparison of these simulations is useful to assess the effects of an altered AGN sub-grid model on the low redshift Lyman-α\alpha Forest. We find significant differences in the IGM temperature-density relation between the two simulations due to changes in the gas heating rate due to AGN. We investigate Lyman-α\alpha Forest observables such as the column density distribution function, flux PDF, and Doppler width (bb-parameter) distribution. Due to the AGN radio mode model, the original Illustris simulations have a factor of 2-3 fewer absorbers than TNG at column densities NHI<1015.5N_{\rm HI}< 10^{15.5} cm−2^{-2}. We show that TNG is in much better agreement with the observed z=0.1z=0.1 flux power spectrum than Illustris. The differences in the amplitude and shape of the flux PDF and power spectrum between Illustris and TNG cannot be attributed to simple changes in the photoheating rate. We also compare the simulated Forest statistics to UV data from the Cosmic Origins Spectrograph (COS) and find that neither simulation can reproduce the slope of the absorber distribution. Both Illustris and TNG also produce significantly smaller bb-parameter distributions than observed in the COS data, possibly due to unresolved or missing sources of turbulence.Comment: Submitted to ApJL, comments welcom

    An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low Redshift Lyman-α\alpha Forest

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    We explore the role of galactic feedback on the low redshift Lyman-α\alpha (Lyα\alpha)~forest (zâ‰Č2z \lesssim 2) statistics and its potential to alter the thermal state of the intergalactic medium. Using the Cosmology and Astrophysics with Machine Learning Simulations (CAMELS) suite, we explore variations of the AGN and stellar feedback models in the IllustrisTNG and Simba sub-grid models. We find that both AGN and stellar feedback in Simba play a role in setting the Lyα\alpha forest column density distribution function (CDD) and the Doppler width (bb-value) distribution. The Simba AGN jet feedback mode is able to efficiently transport energy out to the diffuse IGM causing changes in the shape and normalization of the CDD and a broadening of the bb-value distribution. We find that stellar feedback plays a prominent role in regulating supermassive black hole growth and feedback, highlighting the importance of constraining stellar and AGN feedback simultaneously. In IllustrisTNG, the AGN feedback variations explored in CAMELS do not affect the Lyα\alpha forest, but varying the stellar feedback model does produce subtle changes. Our results imply that the low-zz Lyα\alpha forest can be sensitive to changes in the ultraviolet background (UVB), stellar and black hole feedback, and that AGN jet feedback in particular can have a strong effect on the thermal state of the IGM.Comment: 26 pages, 11 figures, 2 tables, submitted to Ap

    Acute vasoreactivity testing in pediatric idiopathic pulmonary arterial hypertension:an international survey on current practice

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    The aim of this study was to determine practice patterns and inter-institutional variability in how acute vasoreactivity testing (AVT) is performed and interpreted in pediatrics throughout the world. A survey was offered to physicians affiliated with the Pediatric & Congenital Heart Disease Taskforce of the Pulmonary Vascular Research Institute (PVRI), the Pediatric Pulmonary Hypertension Network (PPHNET), or the Spanish Registry for Pediatric Pulmonary Hypertension (REHIPED), from February to December 2016. The survey requested data about the site-specific protocol for AVT and subsequent management of pediatric patients with idiopathic pulmonary arterial hypertension (IPAH) or heritable PAH (HPAH). Twenty-eight centers from 13 countries answered the survey. AVT is performed in most centers using inhaled nitric oxide (iNO). Sitbon criteria was used in 39% of the centers, Barst criteria in 43%, and other criteria in 18%. First-line therapy for positive AVT responders in functional class (FC) I/II was calcium channel blocker (CCB) in 89%, but only in 68% as monotherapy. Most centers (71%) re-evaluated AVT-positive patients hemodynamics after 6-12 months; 29% of centers re-evaluated based only on clinical criteria. Most centers (64%) considered a good response as remaining in FC I or II, with near normalization of pulmonary arterial pressure and pulmonary vascular resistance, but a stable FC I/II alone was sufficient criteria in 25% of sites. Protocols and diagnostic criteria for AVT, and therapeutic approaches during follow-up, were highly variable across the world. Reported clinical practice is not fully congruent with current guidelines, suggesting the need for additional studies that better define the prognostic value of AVT for pediatric IPAH patients

    Unjamming and cell shape in the asthmatic airway epithelium

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    From coffee beans flowing in a chute to cells remodelling in a living tissue, a wide variety of close-packed collective systems— both inert and living—have the potential to jam. The collective can sometimes flow like a fluid or jam and rigidify like a solid. The unjammed-to-jammed transition remains poorly understood, however, and structural properties characterizing these phases remain unknown. Using primary human bronchial epithelial cells, we show that the jamming transition in asthma is linked to cell shape, thus establishing in that system a structural criterion for cell jamming. Surprisingly, the collapse of critical scaling predicts a counter-intuitive relationship between jamming, cell shape and cell–cell adhesive stresses that is borne out by direct experimental observations. Cell shape thus provides a rigorous structural signature for classification and investigation of bronchial epithelial layer jamming in asthma, and potentially in any process in disease or development in which epithelial dynamics play a prominent role
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