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We report Mopra (ATNF), Anglo-Australian Telescope, and Atacama Submillimeter Telescope Experiment observations of a molecular core in Carina, BY72 = G286.21+0.17, which give evidence of large-scale gravitational infall in the dense gas. From the millimetre and far-infrared data, the core has mass ∼ 5,000 M⊙, luminosity ∼ 2–3×10 4 L⊙, diameter ∼ 0.9 pc, and mass infall rate ∼ 2.4×10 −2 M⊙yr −1. If confirmed, this rate for gravitational infall in a molecular core may be the highest yet seen. The near-infrared K-band imaging shows an adjacent compact HII region and IR cluster surrounded by a shell-like photodissociation region showing H2 emission. At the molecular infall peak, the K imaging also reveals a deeply embedded group of stars with associated H2 emission. The combination of these features is very unusual and we suggest they indicate the ongoing formation of a massive star cluster. We discuss the implications of these data for competing theories of massive star formation.
More aggressive therapy has been suggested for patients who have a non-Q wave myocardial infarction (MI) because of the frequency of subsequent unstable angina, recurrent MI, and high mortality rate compared to patients with Q wave MI. The present study was undertaken to investigate the effect of coronary angioplasty on regional myocardial function of the infarct zone in patients with angina early after a non-Q wave MI. The study population consisted of 36 patients undergoing successful coronary angioplasty within 30 days of a non-Q wave MI, in whom sequential left ventricular anglograms of adequate quality were obtained before the initial procedure and at follow-up angiography. The global ejection fraction increased significantly from 60 ± 9% to 67 ± 6% (p = 0.0003). This significant increase in the global ejection fraction was primarily due to a significant improvement in the regional myocardial function of the infarct zone. The results of the present study show not only that ischemic attacks early after a non-Q wave MI may lead to prolonged regional myocardial dysfunction but more important that this depressed myocardium has the potential to achieve normal contraction after successful coronary angioplasty.
Wire-arc directed energy deposition (DED-Arc), also known as wire arc additive manufacturing (WAAM), brings about new opportunities for construction decarbonisation and automation. Overall, the mechanical behaviour of DED-Arc steel is largely comparable to conventionally produced structural steel; however, the performance under tensile loading has been shown to be more variable and susceptible to printing defects. Therefore, an experimental study has been conducted to offer deeper insights into the tensile behaviour of DED-Arc steel elements, with a particular focus on the influence of the process parameters and the consequences of common printing problems. Two groups of DED-Arc steel members with I-section profiles were examined. The first group was designed with different wall thicknesses ranging from 3.5 to 8 mm, achieved by varying key printing parameters and toolpaths, as well as with passive or active cooling. The second group featured the same process parameters but with common printing problems intentionally introduced, including layer shifts, unstable shielding gas, wire feed issues, inclusions, lack of preheating and inconsistent stick out. The test specimens were laser scanned to examine their dimensional properties and surface texture, and then loaded to fracture under axial tension. The influence of wall thickness, toolpath and cooling method on the strength and ductility was highlighted. The common printing problems were shown to slightly deteriorate the strength but significantly reduce the ductility, with unstable shield gas and wire feed issues being the most detrimental. These findings mark a crucial step towards the safe use of DED-Arc for load-bearing applications in construction. • Tensile testing of DED-Arc I-section members printed using ER90S-D2 steel wire was conducted. • Influence of wall thickness, toolpath, cooling method and printing problem was investigated. • A method to characterise surface roughness of DED-Arc from 3D scan data was proposed. • Tensile members showed lower strengths and earlier loss of stiffness compared with coupons. • Printing problems mainly impaired ductility, with shield gas and wire feed issues being the most detrimental.