No abstract is provided for this article.
"Platelet-activating Factor: Role in Pulmonary Injury and Dysfunction and Blood Abnormalities." American Review of Respiratory Disease, 145(3), pp. 726–731
No abstract is provided for this article.
We present multi-wavelength data on the globally infalling molecular cloud/protostellar cluster BYF 73. These include new far-IR spectral line and continuum data from SOFIA's Far Infrared Field-Imaging Line Spectrometer (FIFI-LS), mid-infrared (MIR) observations with the Thermal-Region Camera Spectrograph (T-ReCS) on Gemini-South, and 3 mm continuum data from the Australia Telescope Compact Array (ATCA), plus archival data from Spitzer/IRAC, and Herschel/PACS and SPIRE. The FIFI-LS spectroscopy in [OI]$\lambda63 \mu$m, [OIII]$\lambda88 \mu$m, [OI]$\lambda145 \mu$m, and [CII]$\lambda158 \mu$m highlights different gas environments in and between the dense molecular cloud and HII region. The photo-dissociation region (PDR) between the cloud and HII region is best traced by [OI]$\lambda145 \mu$m and may have density $>$10$^{10}$ m$^{-3}$, but the observed $\lambda145\mu$m/$\lambda63\mu$m and $\lambda63\mu$m/$\lambda158\mu$m line ratios in the densest gas are well outside model values. The HII region is well-traced by [CII], with the $\lambda158\mu$m/$\lambda145\mu$m line ratio indicating a density of 10$^{8.5}$ m$^{-3}$ and a relatively weak ionizing radiation field, 1.5 $\lesssim$ log$(G/G_0)\lesssim$ 2. The T-ReCS data reveal eight protostellar objects in the cloud, of which six appear deeply embedded ($A_V$ $>$ 30$^m$ or more) near the cloud's center. MIR 2 has the most massive core at $\sim$240 M$_{\odot}$, more massive than all the others combined by up to tenfold, with no obvious gas outflow, negligible cooling line emission, and $\sim3-8$% of its 4.7$\times$10$^3$ L$_{\odot}$ luminosity originating from the release of gravitational potential energy. MIR 2's dynamical age may be as little as 7000 yr. This fact, and the cloud's total embedded stellar mass being far less than its gas mass, confirm BYF 73's relatively early stage of evolution.
No abstract is provided for this article.
No abstract is provided for this article.
The behaviour and design of high strength steel (HSS) beams are addressed in the present study. Six in-plane three-point bending tests on three different welded I-sections − two homogeneous S690 steel welded I-sections and one hybrid welded I-section with S690 steel flanges and an S355 steel web, were first conducted. The beam tests were carried out in major axis bending and a bespoke restraint system was designed and employed in the test programme to prevent lateral-torsional buckling. Following the experimental investigation, a thorough finite element (FE) modelling programme was performed, which included a validation study confirming the accuracy of the developed FE models in replicating the flexural behaviour of HSS welded I-section beams, and a parametric study generating additional FE data on HSS welded I-section beams over a broader range of cross-sectional slendernesses, steel grades and loading configurations. The test results obtained in the present study and collected from the literature, together with the generated FE data from the parametric study, were used to evaluate the suitability of the current Eurocode 3 cross-section slenderness limits for HSS homogeneous and hybrid welded I-sections in bending. It is shown that the current Eurocode Class 2 and Class 3 slenderness limits are suitable for the classification of the outstand flange (in compression) and internal web (in bending) elements of both HSS homogeneous and hybrid welded I-sections subjected to major axis bending, while stricter Class 1 slenderness limits are considered necessary to achieve sufficient rotation capacity for plastic design. The findings from the present study indicate that plastic design can be used for HSS structures, provided the proposed stricter Class 1 slenderness limits are employed.