Paris, Cabinet des Medailles, 542: CUP; DOURIS; (continued) BELL KRATER AND DRINKING HORN, MAENAD WITH KROTALA, HERA, SEATED ON CHAIR, WITH PHIALE AND LOTUS SCEPTRE, PROMETHEUS WITH SCEPTRE (BOTH NAMED), MEN, ONE DRAPED, YOUTHS WITH SKYPHOS, LYRE, CUPS AND STAFF, RETURN OF HEPHAISTOS, WITH AXE, DIONYSOS WITH DRINKING HORN, SATYRS WITH HAMMER, PIPES, PIPES CASE [Beazley Archive Vase] (11.91)
Berlin, Schloss Charlottenburg, F1722: COLUMN-KRATER; PROMETHEUS PAINTER, TYRRHENIAN GROUP; HORSEMEN, PROMETHEUS, TIED ON POST, HERAKLES SHOOTING ARROWS, EAGLE, DRAPED MAN WITH STAFF [Beazley Archive Vase] (11.52)
Deepdene, Hope: CALYX-KRATER; DINOS PAINTER; DRAPED YOUTHS, PROMETHEUS IN PATTERNED CHITON, WITH STAFF (?), SATYRS, ONE OLD, ALL WITH TORCHES [Beazley Archive Vase] (10.07)
ARTIST UNKNOWN Artist, Philippe MICHELANGELO After; Prometheus and the vulture: Francesco BARTOLOZZI Engraver; Prometheus and the vulture [Text] (5.89)
Lipchitz, Jacques; Sculptures, sculpture: Prometheus Strangling the Vulture II: Lipchitz, Jacques, PROMETHEUS STRANGLING THE VULTURE II, (1944/1953), bronze, Collection Walker Art Center, Gift of the T.B. Walker Foundation, 1956 [Image] (5.42)
Barefoot, Benjamin F.; Byron's conception of Prometheus /--by Benjamin F. Barefoot.: Thesis (M.A.)--University of North Carolina at Chapel Hill., Bibliography: leaves 3l-32. [Text] (7.27)
Shelley, Percy Bysshe,--1792-1822, Freeman, Martin Joseph,--1899---ed.; A text of Shelley's Prometheus unbound /--by Martin Joseph Freeman.: The editor's thesis--University of Chicago., Bibliography: leaves 338-340. [Text] (3.66)
Fazio, Steven Charles.; The costume of Greek tragedy in the fifth century and in Aeschylus' Prometheus Bound and The Persians.: Thesis (M.A.)-Ohio State University., Bibliography: leaves 47-49. [Text] (2.29)
Bazan, Grant, Arnett, David; Two-Dimensional Hydrodynamics of Pre-Core Collapse: Oxygen Shell Burning: By direct hydrodynamic simulation, using the Piecewise Parabolic Method (PPM) code PROMETHEUS, we study the properties of a convective oxygen burning shell in a SN 1987A progenitor star prior to collapse. The convection is too heterogeneous and dynamic to be well approximated by one-dimensional diffusion-like algorithms which have previously been used for this epoch. Qualitatively new phenomena are seen. The simulations are two-dimensional, with good resolution in radius and angle, and use a large (90-degree) slice centered at the equator. The microphysics and the initial model were carefully treated. Many of the qualitative features of previous multi-dimensional simulations of convection are seen, including large kinetic and acoustic energy fluxes, which are not accounted for by mixing length theory. Small but significant amounts of carbon-12 are mixed non-uniformly into the oxygen burning convection zone, resulting in hot spots of nuclear energy production which are more than an order of magnitude more energetic than the oxygen flame itself. Density perturbations (up to 8%) occur at the edges' of the convective zone and are the result of gravity waves generated by interaction of penetrating flows into the stable region. Perturbations of temperature and electron fraction at the base of the convective zone are of sufficient magnitude to create angular inhomogeneities in explosive nucleosynthesis products, and need to be included in quantitative estimates of yields. Combined with the plume-like velocity structure arising from convection, the perturbations will contribute to the mixing of nickel-56 throughout supernovae envelopes. Runs of different resolution, and angular extent, were performed to test the robustness of these, Comment: For mpeg movies of these simulations, see http://www.astrophysics.arizona.edu/movies.html Submitted to the Astrophysical Journal [Text] [View with Perseus links] (0.75)