Henri Temianka Correspondence; (kubelik)

This collection contains material pertaining to the life, career, and activities of Henri Temianka, violin virtuoso, conductor, music teacher, and author. Materials include correspondence, concert programs and flyers, music scores, photographs, and books.https://digitalcommons.chapman.edu/temianka_correspondence/3850/thumbnail.jp

Henri Temianka Correspondence; (kubelik)

This collection contains material pertaining to the life, career, and activities of Henri Temianka, violin virtuoso, conductor, music teacher, and author. Materials include correspondence, concert programs and flyers, music scores, photographs, and books.https://digitalcommons.chapman.edu/temianka_correspondence/4047/thumbnail.jp

Map of Plasmid pRAL1.

Map of Plasmid pRAL1

Wait times among patients with symptomatic carotid artery stenosis requiring carotid endarterectomy for stroke prevention

BackgroundCurrent Canadian and international guidelines suggest patients with transient ischemic attack (TIA) or nondisabling stroke and ipsilateral internal carotid artery stenosis of 50% to 99% should be offered carotid endarterectomy (CEA) ≤2 weeks of the incident TIA or stroke. The objective of the study was to identify whether these goals are being met and the factors that most influence wait times.MethodsPatients who underwent CEA at the Ottawa Hospital for symptomatic carotid artery stenosis from 2008 to 2010 were identified. Time intervals based on the dates of initial symptoms, referral to and visit with a vascular surgeon, the decision to operate, and the date of surgery were recorded for each patient. The influence of various factors on wait times was explored, including age, sex, type of index event, referring physician, distance from the surgical center, degree of stenosis, and surgeon assigned.ResultsOf the 117 patients who underwent CEA, 92 (78.6%) were symptomatic. The median time from onset of symptoms to surgery for all patients was 79 days (interquartile range [IQR], 34-161). The shortest wait times were observed in stroke patients (49 [IQR, 27-81] days) and inpatient referrals (66 [IQR, 25-103] days). Only 7 of the 92 symptomatic patients (8%) received care within the recommended 2 weeks. The median surgical wait time for all patients was 14 days (IQR, 8-25 days). In the multivariable analysis, significant predictors of longer wait times included retinal TIA (P = .003), outpatient referrals (P = .004), and distance from the center (P = .008). Patients who presented to the emergency department had the shortest delays in seeing a vascular surgeon and subsequently undergoing CEA (P < .0001). There was no difference between surgeons for wait times to be seen in the clinic; however, there were significant differences among surgeons once the decision was made to proceed with CEA.ConclusionsOur wait times for CEA currently do not fall within the recommended 2-week guideline nor does it appear feasible within the current system. Important factors contributing to delays include outpatient referrals, living farther from the hospital, and presenting with a retinal TIA (amaurosis fugax). Our findings also suggest better scheduling practices once a decision is made to operate can modestly improve overall and surgical wait times for CEA

Identifiable Acetylene Features Predicted for Young Earth-like Exoplanets with Reducing Atmospheres Undergoing Heavy Bombardment

The chemical environments of young planets are assumed to be largely influenced by the impacts of bodies lingering on unstable trajectories after the dissolution of the protoplanetary disk. We explore the chemical consequences of impacts within the context of reducing planetary atmospheres dominated by carbon monoxide, methane, and molecular nitrogen. A terawatt high-power laser was selected in order to simulate the airglow plasma and blast wave surrounding the impactor. The chemical results of these experiments are then applied to a theoretical atmospheric model. The impact simulation results in substantial volume mixing ratios within the reactor of 5% hydrogen cyanide (HCN), 8% acetylene (C2H2), 5% cyanoacetylene (HC3N), and 1% ammonia (NH3). These yields are combined with estimated impact rates for the early Earth to predict surface boundary conditions for an atmospheric model. We show that impacts might have served as sources of energy that would have led to steady-state surface quantities of 0.4% C2H2, 400 ppm HCN, and 40 ppm NH3. We provide simulated transit spectra for an Earth-like exoplanet with this reducing atmosphere during and shortly after eras of intense impacts. We predict that acetylene is as observable as other molecular features on exoplanets with reducing atmospheres that have recently gone through their own "heavy bombardments," with prominent features at 3.05 and 10.5 μm

Phylogenetic Analysis of the Complete Mitochondrial Genome of Madurella mycetomatis Confirms Its Taxonomic Position within the Order Sordariales

Background: Madurella mycetomatis is the most common cause of human eumycetoma. The genus Madurella has been characterized by overall sterility on mycological media. Due to this sterility and the absence of other reliable morphological and ultrastructural characters, the taxonomic classification of Madurella has long been a challenge. Mitochondria are of monophyletic origin and mitochondrial genomes have been proven to be useful in phylogenetic analyses. Results: The first complete mitochondrial DNA genome of a mycetoma-causative agent was sequenced using 454 sequencing. The mitochondrial genome of M. mycetomatis is a circular DNA molecule with a size of 45,590 bp, encoding for the small and the large subunit rRNAs, 27 tRNAs, 11 genes encoding subunits of respiratory chain complexes, 2 ATP synthase subunits, 5 hypothetical proteins, 6 intronic proteins including the ribosomal protein rps3. In phylogenetic analyses using amino acid sequences of the proteins involved in respiratory chain complexes and the 2 ATP synthases it appeared that M. mycetomatis clustered together with members of the order Sordariales and that it was most closely related to Chaetomium thermophilum. Analyses of the gene order showed that within the order Sordariales a similar gene order is found. Furthermore also the tRNA order seemed mostly conserved. Conclusion: Phylogenetic analyses of fungal mitochondrial genomes confirmed that M. mycetomatis belongs to the order of Sordariales and that it was most closely related to Chaetomium thermophilum, with which it also shared a comparable gene and tRNA order

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