162,539 research outputs found
5. Schaerer [René). La question platonicienne. Étude sur les rapports de la pensée et de l'expression dans les dialogues. Neuchatel, et Paris, Vrin, 1938
No full textPicard J. G. 5. Schaerer [René). La question platonicienne. Étude sur les rapports de la pensée et de l'expression dans les dialogues. Neuchatel, et Paris, Vrin, 1938. In: Revue des Études Grecques, tome 57, fascicule 269-273,1944. pp. 269-272
5. Schaerer [René). La question platonicienne. Étude sur les rapports de la pensée et de l'expression dans les dialogues. Neuchatel, et Paris, Vrin, 1938
No full textPicard J. G. 5. Schaerer [René). La question platonicienne. Étude sur les rapports de la pensée et de l'expression dans les dialogues. Neuchatel, et Paris, Vrin, 1938. In: Revue des Études Grecques, tome 57, fascicule 269-273,1944. pp. 269-272
C. Favarger, J. Gabus, M. Erard, F. Clerc, Ch. Guyot, R. Schaerer, Ph. H. Menoud, L'Homme face à la Mort. Neuchâtel et Paris, Delachaux et Niestlé, 1952
No full textMehl Roger. C. Favarger, J. Gabus, M. Erard, F. Clerc, Ch. Guyot, R. Schaerer, Ph. H. Menoud, L'Homme face à la Mort. Neuchâtel et Paris, Delachaux et Niestlé, 1952. In: Revue d'histoire et de philosophie religieuses, 33e année n°3,1953. pp. 277-278
[Report to Chief J. E. Curry, by an unknown author #1]
No full textReport to Chief J. E. Curry, by an unknown author. The report contains a list of officers who gave depositions to the United States Attorney
[Report to Chief J. E. Curry, by an unknown author #2]
No full textReport to Chief J. E. Curry, by an unknown author. The report contains a list of officers who gave depositions to the United States Attorney
Realistic ionizing fluxes for young stellar populations from 0.05 to 2 ZÔ
No full textWe present a new grid of ionizing fluxes for O and Wolf–Rayet (W–R) stars for use with evolutionary synthesis codes and single-star H ii region analyses. A total of 230 expanding, non-LTE, line-blanketed model atmospheres have been calculated for five metallicities (0.05, 0.2, 0.4, 1 and 2 Z⊙) using the wm-basic code of Pauldrach, Hoffmann & Lennon for O stars and the cmfgen code of Hillier & Miller for W–R stars. The stellar wind parameters are scaled with metallicity for both O and W–R stars. We compare the ionizing fluxes of the new models with the CoStar models of Schaerer & de Koter and the pure helium W–R models of Schmutz, Leitherer & Gruenwald. We find significant differences, particularly above 54 eV, where the emergent flux is determined by the wind density as a function of metallicity. The new models have lower ionizing fluxes in the He i continuum with important implications for nebular line ratios. We incorporate the new models into the evolutionary synthesis code starburst99 and compare the ionizing outputs for an instantaneous burst and continuous star formation with the work of Schaerer & Vacca (SV98), and Leitherer et al. The changes in the output ionizing fluxes as a function of age are dramatic. We find that, in contrast to previous studies, nebular He ii λ4686 will be at, or just below, the detection limit in low metallicity starbursts during the W–R phase. The new models have lower fluxes in the He i continuum for Z≥ 0.4 Z⊙ and ages ≤7 Myr because of the increased line blanketing. We test the accuracy of the new model atmosphere grid by constructing photoionization models for simple H ii regions, and assessing the impact of the new ionizing fluxes on important nebular diagnostic line ratios. For the case of an H ii region where the ionizing flux is given by the WM-basic dwarf O star grid, we show that He iλ5786/Hβ decreases between 1 and 2 Z⊙ in a similar manner to observations. We find that this decline is caused by the increased effect of line blanketing above solar metallicity. We therefore suggest that a lowering of the upper mass limit at high abundances is not required to explain the diminishing strength of He iλ5786/Hβ , as has been suggested in the past. For an H ii region where the ionizing flux is provided by an instantaneous burst of total mass 106 M⊙ , we plot the softness parameter η' against the abundance indicator R23 for ages of 1–5 Myr. The new models are coincident with the observational data of Bresolin et al., particularly during the W–R phase, unlike the previous models of SV98 which generally over-predict the hardness of the ionizing radiation
A novel CT-based contrast enhancement technique for markerless lung tumor tracking in X-ray projection images
No full textTime-consistent parametrization from dynamic optical surface detection for respiratory motion recovery in radiation oncology
No full textMurder on the mountain: author talk with Peter J. Wosh
No full textAuthor talk by Peter J. Wosh on May 5th, 2022, on his book, "Murder on the Mountain: crime, passion, and punishment in gilded age New Jersey.
Mr. Melvin J. Collier, RWWL AUC, June 2011
No full textThis video is a conversation with Mr. Melvin J. Collier. Mr. Collier talks about his book, "From Mississippi to Africa: A Journey of Discovery". Daniel Le, AUC Woodruff Library, is the interviewer
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